Modeling gas-surface processes. Theory and Experiments for adsorption energies determination of nitrile / isonitrile isomers.
|
|
- Poppy Goodman
- 6 years ago
- Views:
Transcription
1 Modeling gas-surface processes Theory and Experiments for adsorption energies determination of nitrile / isonitrile isomers. Y. Ellinger, A. Markovits, F. Pauzat, M. Doronin (Laboratoire de Chimie Théorique - LCT) M. Bertin, M. Doronin, J.-H. Fillion (Observatoire de Paris LERMA) M16 by NASA
2 Nitriles and Isonitriles Molecules in the ISM (as of 02/2016) Almost 20% of the ~ 200 organics detected have a CN triple bond. 37 species split in 30 R-CN 7 R-NC If R is saturated the list is reduced to CH 3 CN (Solomon et al 1971) CH 3 CH 2 CN (Johnson et al 1977) n-c 3 H 7 CN and i-c 3 H 7 CN (Belloche et al 2009; 2014) CH 3 NC (Cernicharo et al 1988)
3 Abundance ratios as constraints to chemical models HCN/HNC (the most studied) Variations from ~1 in cold molecular clouds to ~n x 1000 in PDRs CH 3 CN/CH 3 NC Variations negligibles ~50 in all situations Why?
4 Possible reasons Observational bias: Radio observations are blind to molecules depleted on the grains Observational fact: The abundance ratios are different for the gas phase and for the depleted species (Dipole moment: µ ~ 4 D for CH 3 CN/CH 3 NC) Possible origin: Selective adsorption between isomers
5 Interstellar surfaces Original work by Greenberg (1976) Silicates: Molster et al (2002) Water ices: Schutte (1999); Gigg et al (2004) Watanabe & Kouchi (2008); Boogert et al (2015) Carbonaceous matter: Leger & Puget (1984); Allamandola et al (1985); Papoular et al (1995) Experiments TPD: Temperature Programmed Desorption Numerical simulations First principle periodic DFT calculations M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011) M. Bertin, M. Doronin, et al; A&A, 598, A18 (2017) M. Bertin, M. Doronin, et al; A&A, in press (2017)
6 TPD: Temperature Programmed Desorption (ices) Mass spectrometer RAIRS RAIRS H 2 O ice Polycrystalline Au T = 80 K T 1 K.min - 1 Adsorption/desorption behaviours of each isomer Estimation of adsorption energy in the single molecule limit Measure of the ability to bind with water surface via hydrogen bonding
7 Experimental check è adsorption (ices) Vola%les : Below 100 K (H 2, CO, CH 4, CO 2 ) E Ads ~ 0.1 ev Weakly bound : Before H 2 O (HCOOCH 3, CH 3 OCH3...) E Ads ~ 0.3 ev Strongly bound : With H 2 O (CH 3 COOH, CH 3 CH 2 OH...). Adapted from M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011) E Ads ~ 0.6 ev
8 Numerical simulation è adsorption (ices) E (kcal/mol) HOCH 2 CHO 27 [CH 3 COOH] [HCOOCH 3 ] 17 0 HCOOCH 3 CH 3 COOH = 0,01 à 0,1 [CH 3 COOH] [HOCH 2 CHO] = 0,05 E CH3COOH = 17,2 kcal/mol E HOCH2CHO = 11,6 kcal/mol E HCOOCH3 = 7,3 kcal/mol. M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011)
9 Theoretical approaches for weak interactions with systems of large dimensions Ab initio / DFT molecule molecule ρ 1 ρ molecule support support ρ 2 support «supermolecule» approach: è BSSE artifact Tran et al. J. Phys. Chem. B (2002); Heine et al. PCCP (2004) KSCED approach Tran et al. J. Phys. Chem. B (2002) Periodic approach: plane waves
10 Adsorption on graphite Position of R-CN Orientation of RCN L: middle of a bond X X: to plane C: carbon atom O: center of the ring L O C Z Y Y: to plane Z: to plane
11 Periodic approach Vertical replication Vertical replication vacuum
12 Adsorption on graphene: vertical dimension of the cell vertical Dimension (Ǻ) ΔE (kcal/mol) Test of the adsorption energy of a dipolar system: HCN
13 Nitrile versus Isonitrile on perfect graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 275 mev (30 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 255 mev (30 mev) 430 ± 25 mev No significant difference between nitrile and isonitrile on perfect HOPG M. Bertin, M. Doronin, et al; A&A, in press (2017)
14 Nitrile versus Isonitrile on damaged graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 310 mev (40 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 300 mev (40 mev) 430 ± 25 mev No significant difference between nitrile and isonitrile on HOPG with 2C hole defect M. Bertin, M. Doronin, et al; A&A, in press (2017)
15 Nitrile versus Isonitrile on damaged graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 390 mev (50 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 350 mev (50 mev) 430 ± 15 mev No significant difference between nitrile and isonitrile on HOPG with 2C hole hydrogenated defect M. Bertin, M. Doronin, et al; A&A, in press (2017)
16 Nitrile versus Isonitrile on damaged graphite CH3CN Eads (Th) = 480 mev (0 mev) Eads (Exp) 440 ± 25 mev CH3NC Eads (Th) = 440 mev (0 mev) Eads (Exp) 430 ± 25 mev No significant difference between nitrile and isonitrile on HOPG with hydrogenated step defect M. Bertin, M. Doronin, et al; A&A, in press (2017)
17 Nitrile versus Isonitrile on water ice CH 3 CN CH 3 NC E ads (The) E ads (Exp) = 558 mev 565 ± 25 mev E ads (The) E ads (Exp) = 545 mev 540 ± 15 mev No significant difference between nitrile and isonitrile Similar results on silicates M. Bertin, M. Doronin, et al; A&A, 598, A18 (2017)
18 What to conclude Theory Eads (mev) Perfect HOPG C hole CH hole q No significant difference between nitrile and isonitrile whatever substract and defects (within ~10%) q Systemetic shift of E ads towards lower values for CH 3 NC q CH 3 CN/CH 3 NC not affected by environment TPD Eads (mev) CH3CN CH3NC CH3CN CH3NC Step-H ± ± 25 α-quartz (0001) ± ± 25 Water ice (Ih) ± ± 15
19 The End
20 Adsorption of COMs and simulations Bertin, M., Doronin, M., Fillion, F.-H., Michaut, X.,Philippe, L., Lattelais, M., Markovits, A., Pauzat, F.,Ellinger, Y. & Guillemin, J.-C. 2017, A&A, 598, A18 and 2017, A&A, Part II in press Doronin, M., Bertin, M., Michaut, X., Philippe, P., &Fillion, J.-H. 2015, J. Chem. Phys., 143, Lattelais, M., Pauzat, F., Ellinger, Y., & Ceccarelli, C. 2015, A&A, 578, A62 Pauzat, F., Marloie, G., Markovits, A., & Ellinger, Y., 2015, Int.,J. Astro., 14, 563 Lattelais, M., Bertin, M., Mokrane, H., et al. 2011, A&A, 532, A12 Pauzat, F., Lattelais, M., Ellinger, Y., & Minot, C. 2011, MNRAS, 412, 2729
UV photodesorption of intact molecules and of photofragments from solid formaledhyde and methanol
UV photodesorption of intact molecules and of photofragments from solid formaledhyde and methanol Mathieu Bertin, Xavier Michaut, Claire Romanzin, Géraldine Féraud, Pascal Jeseck, Laurent Philippe, Harold
More informationarxiv: v1 [astro-ph.ga] 17 Oct 2016
Astronomy & Astrophysics manuscript no. 29394 langugage edited 2col c ESO 2016 October 18, 2016 arxiv:1610.05010v1 [astro-ph.ga] 17 Oct 2016 Nitrile versus isonitrile adsorption at interstellar grains
More informationNon-thermal ion desorption from nitrilebearing astrophysical ice analogues studied by electron and heavy ion bombardment
Non-thermal ion desorption from nitrilebearing astrophysical ice analogues studied by electron and heavy ion bombardment Fabio Ribeiro, Guilherme C. Almeida, Wania Wolff, Enio Frota da Silveira, Maria
More informationHydrogenation of solid hydrogen cyanide HCN and methanimine CH 2 NH at low temperature
Hydrogenation of solid hydrogen cyanide HCN and methanimine CH 2 NH at low temperature P. Theule, F. Borget, F. Mispelaer, G. Danger, F. Duvernay, J. C. Guillemin, and T. Chiavassa 5 534,A64 (2011) By
More informationTERAHERTZ SPECTROSCOPY OF DEUTERATED ACETALDEHYDE: CH 2 DCHO
TERAHERTZ SPECTROSCOPY OF DEUTERATED ACETALDEHYDE: CH 2 DCHO L. Margulès, R. A. Motiyenko Laboratoire PhLAM, Université de Lille1, France L. H. Coudert LISA, CNRS, Universités Paris Est Créteil et Paris
More informationUniversité de Cergy-Pontoise, FRANCE
Water formation through O 2 +D pathway on cold silicate, graphite and amorphous water surfaces of interstellar interest Henda Chaabouni Marco Minissale, François Dulieu LERMA-LAMAp, UMR 82 du CNRS, Observatoire
More informationChemical modelling of formamide and methyl isocyanate in star-forming regions
Chemical modelling of formamide and methyl isocyanate in star-forming regions David Quénard Post-Doctoral Research Assistant Izaskun Jiménez-Serra (QMUL), Serena Viti (UCL), Jon Holdship (UCL), Audrey
More information2- The chemistry in the. The formation of water : gas phase and grain surface formation. The present models. Observations of molecules in the ISM.
2- The chemistry in the ISM. The formation of water : gas phase and grain surface formation. The present models. Observations of molecules in the ISM. 1 Why studying the ISM chemistry? 1- The thermal balance,
More informationThe rôle of surfaces in prebiotic chemistry. Piero Ugliengo University of Torino Dip. Chimica Via P. Giuria, 7 - Torino
The rôle of surfaces in prebiotic chemistry Piero Ugliengo University of Torino Dip. Chimica Via P. Giuria, 7 - Torino 1 A collaborative work Dip. Chimica - NIS Centre Torino University TO BCN Dep. Quimica
More informationSurfaces processes. François Dulieu LERMA. Paris Observatory and Cergy Pontoise University
Surfaces processes François Dulieu LERMA Paris Observatory and Cergy Pontoise University Cold surfaces and astrophysics Image credit: J. Freitag and S. Messenger Smoky areas = dust grains Cold (10-15 K)
More informationPhysical Chemistry Chemical Physics
Physical Chemistry Chemical Physics www.rsc.org/pccp Volume 12 Number 23 21 June 2010 Pages 5929 6292 ISSN 1463-9076 COVER ARTICLE Brown et al. Ice in space: surface science investigations of the thermal
More informationESO in the 2020s: Astrobiology
ESO in the 2020s: Astrobiology Izaskun Jimenez-Serra (IIF Marie Curie Fellow, ESO) Leonardo Testi (ESO), Paola Caselli (MPE) & Serena Viti (UCL) 1 From the ISM to the Origin of Life Molecular clouds (Pre-stellar
More informationFirst-principles Studies of Formaldehyde Molecule Adsorption on Graphene Modified with Vacancy, -OH, -CHO and -COOH Group
2017 Asia-Pacific Engineering and Technology Conference (APETC 2017) ISBN: 978-1-60595-443-1 First-principles Studies of Formaldehyde Molecule Adsorption on Graphene Modified with Vacancy, -OH, -CHO and
More informationOxygen Chemistry on Dust Grains
Oxygen Chemistry on Dust Grains Gianfranco Vidali and Jiao He, Tyler Hopkins, Jianming Shi Syracuse University Syracuse, NY (USA) Jean Louis Lemaire Paris Observatoire, Paris (France) Michael Kaufman San
More informationatoms H. * Infrared **Optical l - linear c-cyclic
2 3 4 5 6 7 atoms H *,* 2 C 3 * c-c 3 H C 5 * C 5 H C 6 H AlF C 2 H l-c 3 H C 4 H l-h 2 C 4 CH 2 CHCN AlCl C 2 O C 3 N C 4 Si C 2 H 4 CH 3 C 2 H C 2 ** C 2 S C 3 O l-c 3 H 2 CH 3 CN HC 5 N CH CH 2 C 3
More informationCO and N2 differential depletion in prestellar cores: Experimental study of N2 desorption induced by the CO presence on ices
CO and N2 differential depletion in prestellar cores: Experimental study of N2 desorption induced by the CO presence on ices T.Nguyen, S. Baouche, E.Congiu, H.Chaabouni, L.Pagani, and F.Dulieu LERMA Lamap,
More informationOrtho-para transitions of molecular hydrogen in H + + H 2 collisions. Tomás González Lezana
Ortho-para transitions of molecular hydrogen in H + + H 2 collisions Tomás González Lezana Dep. de Física Atómica, Molecular y de Agregados Instituto de Física Fundamental (CSIC) MADRID (ESPAÑA) Grenoble
More informationDensity functional theory with an approximate kinetic energy functional applied to study structure and stability of weak van der Waals complexes
JOURNAL OF CHEMICAL PHYSICS VOLUME 108, NUMBER 15 15 APRIL 1998 Density functional theory with an approximate kinetic energy functional applied to study structure and stability of weak van der Waals complexes
More informationMethyl Formate as a probe of temperature and structure of Orion-KL
Methyl Formate as a probe of temperature and structure of Orion-KL Cécile Favre Århus University - Institut for Fysik og Astronomy (IFA) N. Brouillet (LAB), D. Despois (LAB), A. Baudry (LAB), A. Wootten
More informationLLNL-PRES W. M. Howard and S. Bastea Extreme Chemistry Group. Lawrence Livermore National Laboratory
Titan s Interior :(I) A thermo-chemical assessment suggests N 2 is the dominate source of nitrogen near Titan s surface\\ and (II) future studies on the effects of comet impacts on organic and surface
More information8: Composition and Physical state of Interstellar Dust
8: Composition and Physical state of Interstellar Dust James Graham UC, Berkeley 1 Reading Tielens, Interstellar Medium, Ch. 5 Mathis, J. S. 1990, AARA, 28, 37 Draine, B. T., 2003, AARA, 41, 241 2 Nature
More informationInterstellar chemistry. Liv Hornekær
Interstellar chemistry Liv Hornekær Overall structure of the ISM 21 cm 2.6 mm Overview picture 21 cm observations Leiden-Dwingeloo/Argentina/Bonn H atom La: 121.6 nm, 10.2 ev J=L+S F=I+J Relative abundance
More informationAmandeep S. Bolina, Angela J. Wolff, and Wendy A. Brown*
16836 J. Phys. Chem. B 2005, 109, 16836-16845 Reflection Absorption Infrared Spectroscopy and Temperature-Programmed Desorption Studies of the Adsorption and Desorption of Amorphous and Crystalline Water
More informationMoment equations for chemical reactions on interstellar dust grains. A. Lipshtat and O. Biham
A&A 400, 585 593 (003) DOI: 10.1051/0004-6361:00190 c ESO 003 Astronomy & Astrophysics Moment equations for chemical reactions on interstellar dust grains A. Lipshtat and O. Biham Racah Institute of Physics,
More informationNucleosynthesis and stellar lifecycles. A. Ruzicka
Nucleosynthesis and stellar lifecycles A. Ruzicka Stellar lifecycles A. Ruzicka Outline: 1. What nucleosynthesis is, and where it occurs 2. Molecular clouds 3. YSO & protoplanetary disk phase 4. Main Sequence
More informationAstrochemistry (2) Interstellar extinction. Measurement of the reddening
Measurement of the reddening The reddening of stellar colours casts light on the properties of interstellar dust Astrochemistry (2) Planets and Astrobiology (2016-2017) G. Vladilo The reddening is measured
More informationAdvanced Electronic Structure Theory Density functional theory. Dr Fred Manby
Advanced Electronic Structure Theory Density functional theory Dr Fred Manby fred.manby@bris.ac.uk http://www.chm.bris.ac.uk/pt/manby/ 6 Strengths of DFT DFT is one of many theories used by (computational)
More information" There's life Jim...but we don't KNOW it (yet): a journey through the chemically controlled cosmos from star birth to the formation of life"
" There's life Jim...but we don't KNOW it (yet): a journey through the chemically controlled cosmos from star birth to the formation of life" 30 th May 2007, Stockholm Observatory with support from the
More informationDissociative recombination reactions. Wolf D. Geppert ISSI workshop, Bern (CH) December 2008
Dissociative recombination reactions Wolf D. Geppert ISSI workshop, Bern (CH) December 2008 Important electron-ion processes A B - Resonant ion pair formation (high energies) AB hν Radiative recombination
More informationFormation of complex molecules after energetic processing of icy grain mantles
Formation of complex molecules after energetic processing of icy grain mantles Maria Elisabetta Palumbo INAF Osservatorio Astrofisico di Catania mepalumbo@oact.inaf.it http://www.oact.inaf.it/weblab/ Molecules
More informationE. Rauls. Department of Theoretical Physics, Faculty of Natural Sciences, University of Paderborn, D Paderborn, Germany;
The Astrophysical Journal, 679:531Y536, 2008 May 20 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. A CATALYZED ROUTES TO MOLECULAR HYDROGEN FORMATION AND HYDROGEN ADDITION
More informationOxidation processes on cold surfaces, diffusion and reactivity
Marco Minissale Université de Cergy-Pontoise and Observatoire de Paris Oxidation processes on cold surfaces, diffusion and reactivity Leiden, 13th March 2013 What we know about oxygenation? Astrophysical
More informationA laboratory study of the OD stretching mode band in H 2 O:HDO ice mixtures.
A laboratory study of the OD stretching mode band in H 2 O:HDO ice mixtures. Preliminary Results R.G. Urso 1,2, C. Scirè 1, G.A. Baratta 1, M.E. Palumbo 1 rurso@oact.inaf.it 1 INAF-Osservatorio Astrofisico
More informationCARBON MONOXIDE ENTRAPMENT IN INTERSTELLAR ICE ANALOGS M. P. Collings, J. W. Dever, H. J. Fraser, 1 M. R. S. McCoustra, and D. A.
The Astrophysical Journal, 583:1058 1062, 2003 February 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. CARBON MONOXIDE ENTRAPMENT IN INTERSTELLAR ICE ANALOGS M. P.
More information* Corresponding authors:
Mechanism of Olefin Hydrogenation Catalysis Driven by Palladium-Dissolved Hydrogen Satoshi Ohno,*, Markus Wilde,*, Kozo Mukai, Jun Yoshinobu, and Katsuyuki Fukutani Institute of Industrial Science, The
More informationAdsorption on Interstellar Analog Surfaces: from Atoms to Organic Molecules
THÈSE DE DOCTORAT DE L UNIVERSITÉ PIERRE ET MARIE CURIE Spécialité : Physique École doctorale : Physique en Île-de-France réalisée au Laboratoire d Études du Rayonnement et de la Matière en Astrophysique
More informationReduction of unsaturated compounds under interstellar conditions: chemoselective reduction of C C and C=C bonds over C=O functional group
Reduction of unsaturated compounds under interstellar conditions: chemoselective reduction of C C and C=C bonds over C=O functional group Mindaugas Jonusas, Jean-Claude Guillemin, Lahouari Krim To cite
More informationWork hard. Be nice. Name: Period: Date:
Name: Period: Date: UNIT 6: Organic Chemistry Lesson 2: Isomers and Side Chains By the end of today, you will have an answer to: What happens when two different molecules have the same formula? Do Now:
More information10 Marking scheme: End-of-chapter test
1 a Element Carbon Hydrogen Oxygen Percentage 62.1 10.3 27.6 Mass in 100 g 62.1 g 10.3 g 27.6 g Number of moles 62.1 10.3 27.6 = 5.18 = 10.3 = Relative number 5.18 10.3 of atoms = 3 = 6 = 1 empirical formula
More informationAstrochemistry Lecture 2 Basic Processes (cont d)
Astrochemistry Lecture 2 Basic Processes (cont d) Ewine F. van Dishoeck Leiden Observatory Spring 2008 Types of chemical reactions Formation of bonds Radiative association: X + + Y XY + + hν Associative
More informationThe structure of water on the (0001) surface of graphite
Surface Science 532 535 (2003) 166 172 www.elsevier.com/locate/susc The structure of water on the (0001) surface of graphite P. Cabrera Sanfelix a, S. Holloway a, K.W. Kolasinski b, G.R. Darling a, * a
More informationProtonated Polycyclic Aromatic Hydrocarbons and the Interstellar Medium
1 Chapter 1 Protonated Polycyclic Aromatic Hydrocarbons and the Interstellar Medium 1.1 Interstellar Molecules Although hydrogen is the most abundant element in the universe, it is other elements that
More informationSupporting information for Polymer interactions with Reduced Graphene Oxide: Van der Waals binding energies of Benzene on defected Graphene
Supporting information for Polymer interactions with Reduced Graphene Oxide: Van der Waals binding energies of Benzene on defected Graphene Mohamed Hassan, Michael Walter *,,, and Michael Moseler, Freiburg
More informationLecture 11. IR Theory. Next Class: Lecture Problem 4 due Thin-Layer Chromatography
Lecture 11 IR Theory Next Class: Lecture Problem 4 due Thin-Layer Chromatography This Week In Lab: Ch 6: Procedures 2 & 3 Procedure 4 (outside of lab) Next Week in Lab: Ch 7: PreLab Due Quiz 4 Ch 5 Final
More information9 - The Hot Corinos. Complex organic molecules in the inner 100 AU envelope of Solar type protostars
9 - The Hot Corinos Complex organic molecules in the inner 100 AU envelope of Solar type protostars 1 THE COLLAPSING PROTOSTAR PHASE 2 THE INNER ENVELOPES OF LOW MASS PROTOSTARS Direct observations of
More informationEVOLUTION OF MOLECULAR ABUNDANCE IN PROTOPLANETARY DISKS
EVOLUTION OF MOLECULAR ABUNDANCE IN PROTOPLANETARY DISKS Yuri Aikawa 1 Department of Earth and Planetary Science, University of Tokyo, Bunkyo-ku, Tokyo 113, Japan arxiv:astro-ph/9706204v1 19 Jun 1997 Toyoharu
More informationTitle of file for HTML: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References
Title of file for HTML: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References Title of file for HTML: Supplementary Movie 1 Description: This movie
More informationTheoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs
Georgia Southern University From the SelectedWorks of Ryan C. Fortenberry 2013 Theoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs Ryan C. Fortenberry, Georgia Southern
More informationHYDROGENATION OF CO ON PURE SOLID CO AND CO-H 2 O MIXED ICE
The Astrophysical Journal, 616:638 642, 2004 November 20 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. HYDROGENATION OF CO ON PURE SOLID CO AND CO-H 2 O MIXED ICE Naoki
More informationOutline. Introduction: graphene. Adsorption on graphene: - Chemisorption - Physisorption. Summary
Outline Introduction: graphene Adsorption on graphene: - Chemisorption - Physisorption Summary 1 Electronic band structure: Electronic properties K Γ M v F = 10 6 ms -1 = c/300 massless Dirac particles!
More informationEffect of Electric Field on Condensed-Phase Molecular Systems. II. Stark Effect on the Hydroxyl Stretch Vibration of Ice
Effect of Electric Field on Condensed-Phase Molecular Systems. II. Stark Effect on the Hydroxyl Stretch Vibration of Ice Sunghwan Shin, Hani Kang, Daeheum Cho, Jin Yong Lee, *, and Heon Kang *, Department
More informationChem. 1C Midterm 1 Practice Test 2
Chem. 1C Midterm 1 Practice Test 2 First initial of last name Name Student Number All work must be shown on the exam for partial credit. Points will be taken off for incorrect or no units. Calculators
More informationStatus of the Diffuse Interstellar Band Problem
Status of the Diffuse Interstellar Band Problem Ben McCall Department of Chemistry and Department of Astronomy University of Illinois at Urbana-Champaign APO DIB Collaboration: Tom Fishman (Chicago), Scott
More informationRadio astronomy, Lecture 14
Radio astronomy, Lecture 14 1) Molecular clouds 2) Dust 3) ALMA 1937 1 Laboratory tour Helmholtzweg 3 (rotes Haus), Montag 05.02.18 12-00 1937 2 The whole sky (by eyes) Lund observatory 3 The whole sky
More informationGAS PHASE CHEMICAL KINETICS : EXPERIMENTAL ADVANCES AND PROSPECTS
GAS PHASE CHEMICAL KINETICS : EXPERIMENTAL ADVANCES AND PROSPECTS Sébastien Le Picard France Astrophysique de Laboratoire Institut de Physique de Rennes Université de Rennes 1 Gas phase chemistry in the
More informationAstrochimistry Spring 2013
Astrochimistry Spring 2013 Lecture 3: H2 Formation NGC 7023 - HST Julien Montillaud 1st February 2013 Outline I. The most abundant molecule in the Universe (6 p.) I.1 Relative abundances I.2 Historical
More informationTPD-MS. Photocatalytic Studies Using Temperature Programmed Desorption Mass Spectrometry (TPD-MS) APPLICATION NOTE NOTE
TPD-MS APPLICATION NOTE NOTE Photocatalytic Studies Using Temperature Programmed Desorption Mass Spectrometry (TPD-MS) Thermal analysis consists of many techniques for the exploration of the physical properties
More informationAu-C Au-Au. g(r) r/a. Supplementary Figures
g(r) Supplementary Figures 60 50 40 30 20 10 0 Au-C Au-Au 2 4 r/a 6 8 Supplementary Figure 1 Radial bond distributions for Au-C and Au-Au bond. The zero density regime between the first two peaks in g
More informationNew Perspective on structure and bonding in water using XAS and XRS
New Perspective on structure and bonding in water using XAS and XRS Anders Nilsson Stanford Synchrotron Radiation Laboratory (SSRL) and Stockholm University, Sweden R. Ludwig Angew. Chem. 40, 1808 (2001)
More informationPhoto-Dissociation Resonances of Jet-Cooled NO 2 by CW-CRDS
Photo-Dissociation Resonances of Jet-Cooled NO 2 by CW-CRDS Patrick DUPRÉ Laboratoire de Physico-Chimie de l Atmosphère, Université du Littoral, Côte d Opale Dunkerque, France ISMS 22-26 June 2015 Patrick
More informationEffects of methanol on crystallization of water in the deeply super cooled region
Effects of methanol on crystallization of water in the deeply super cooled region Ryutaro Souda Nanoscale Materials Center National Institute for Materials Science Japan PHYSICAL REVIEW B 75, 184116, 2007
More informationInterstellar dust: The hidden protagonist. Stéphanie Cazaux Marco Spaans Vincent Cobut Paola Caselli Rowin Meijerink
Interstellar dust: The hidden protagonist Stéphanie Cazaux Marco Spaans Vincent Cobut Paola Caselli Rowin Meijerink th 15 February 2012 Overview Star form in clouds made of gas + dust Catalyst: Enrich
More informationCOMBINED IRAM, Herschel/HIFI and ALMA STUDIES of abundant molecules in ORION KL
COMBINED IRAM, Herschel/HIFI and ALMA STUDIES of abundant molecules in ORION KL Belén Tercero ICMM-CSIC, Madrid, Spain CONTENTS 1. ORION REGION 2. THREE SETS OF DATA 3. STUDIES OF ORION-KL 4. CONCLUSIONS
More informationList of Figures Page Figure No. Figure Caption No. Figure 1.1.
List of Figures Figure No. Figure Caption Page No. Figure 1.1. Cation- interactions and their modulations. 4 Figure 1.2. Three conformations of benzene dimer, S is not a minimum on the potential energy
More informationMillimeter and submillimeter wave spectra of N-methyl formamide and propionamide
Millimeter and submillimeter wave spectra of N-methyl formamide and propionamide A.A. Mescheryakov, E.A. Alekseev, V.V. Ilyushin Institute of Radio Astronomy, NASU, Kharkov, Ukraine R.A. Motiyenko, L.
More informationSupporting information for Chemical and Electrochemical. Surfaces: Insights into the Mechanism and Selectivity from DFT.
Electronic Supplementary Material (ESI) for RSC Advances. This journal is The Royal Society of Chemistry 2015 Supporting information for Chemical and Electrochemical Hydrogenation of CO 2 to hydrocarbons
More informationSticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
Astronomy & Astrophysics ESO 0 Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions H. Chaabouni, H. Bergeron, S. Baouche, F. Dulieu, E. Matar, E. Congiu, L. Gavilan,
More informationarxiv: v1 [astro-ph] 22 May 2008
Structural effects of ice grain surfaces on the hydrogenation of at low temperatures arxiv:0805.3383v1 [astro-ph] 22 May 2008 H. Hidaka a,, N. Miyauchi a, A. Kouchi a, N. Watanabe a a Institute of Low
More informationAP Chemistry Readiness Liquids, Solids, and Solutions Review Page 1 of 16. AP Chemistry Review Session December 10, 2016 UCLA
AP Chemistry Readiness Liquids, Solids, and Solutions Review Page 1 of 16 AP Chemistry Review Session December 10, 2016 UCLA Michael A. Morgan mmorgan@lausd.net Richard Erdman xchemteach@yahoo.com Francisco
More informationCarbon Compounds. Chemical Bonding Part 2
Carbon Compounds Chemical Bonding Part 2 Introduction to Functional Groups: Alkanes! Alkanes Compounds that contain only carbons and hydrogens, with no double or triple bonds.! Alkyl Groups A part of a
More informationCHEM 301: Homework assignment #12
CHEM 301: Homework assignment #12 Solutions 1. Let s practice converting between wavelengths, frequencies, and wavenumbers. (10%) Express a wavelength of 442 nm as a frequency and as a wavenumber. What
More informationAstrochemistry from a Sub-pc Scale to a kpc Scale. Satoshi Yamamoto Department of Physics and RESCUE The University of Tokyo
Astrochemistry from a Sub-pc Scale to a kpc Scale Satoshi Yamamoto Department of Physics and RESCUE The University of Tokyo Contents Physical and Chemical Processes in Disk Formation around Solar-type
More informationIntroduction. H2 case. The Chemical Desorption. O+O case O2 + H. APiMI meeting Leiden, 13th of march Water form. Others cases.
The Chemical Desorption APiMI meeting Leiden, 13th of march 2013 Accretion time H/H2 transition 3 nn==~~1/cm 1/cm3 T= T=1000K 1000K n > 1000/cm3 T= 10 K n = 100/cm3 Tgas= 100 K Tgrains= 20 K CO depletion
More informationarxiv: v1 [astro-ph] 17 Sep 2007
Astronomy & Astrophysics manuscript no. 8210Hat c ESO 2008 February 1, 2008 H-atom bombardment of CO 2, HCOOH and CH 3 CHO containing ices S. E. Bisschop, G. W. Fuchs, E. F. van Dishoeck, and H. Linnartz
More informationSupporting information for Activity descriptors for CO 2 electroreduction to methane on transition-metal catalysts
Supporting information for Activity descriptors for CO 2 electroreduction to methane on transition-metal catalysts Andrew A. Peterson 1,3, Jens K. Nørskov 1,2 SUNCAT Center for Interface Science and Catalysis,
More informationTHE NITRILES PROJECT: MOLECULE FORMATION IN THE GALACTIC CENTER
THE NITRILES PROJECT: MOLECULE FORMATION IN THE GALACTIC CENTER JOANNA CORBY (www.astro.virginia.edu/~jfc9va) University of Virginia, Department of Astronomy Advised by Anthony Remijan, National Radio
More informationThe effects of methanol on the trapping of volatile ice components
doi:10.1093/mnras/stv109 The effects of methanol on the trapping of volatile ice components Daren J. Burke and Wendy A. Brown Division of Chemistry, University of Sussex, Falmer, Brighton, BN1 9QJ, UK
More informationAstronomy. Astrophysics. Formation of methyl formate after cosmic ion irradiation of icy grain mantles. P. Modica and M. E. Palumbo. 1.
DOI: 10.1051/0004-6361/201014101 c ESO 2010 Astronomy & Astrophysics Formation of methyl formate after cosmic ion irradiation of icy grain mantles P. Modica and M. E. Palumbo INAF Osservatorio Astrofisico
More informationMany-body dispersion interactions between semiconducting wires
Many-body dispersion interactions between semiconducting wires Alston J. Misquitta TCM Group, Cavendish Laboratory University of Cambridge 26 th July, 2010 Collaborators James Spencer (Imperial College,
More informationSupporting Information for. Dynamics Study"
Supporting Information for "CO 2 Adsorption and Reactivity on Rutile TiO 2 (110) in Water: An Ab Initio Molecular Dynamics Study" Konstantin Klyukin and Vitaly Alexandrov,, Department of Chemical and Biomolecular
More informationThermal desorption of water ice in the interstellar medium
Mon. Not. R. Astron. Soc. 327, 1165 1172 (2001) Thermal desorption of water ice in the interstellar medium Helen J. Fraser, 1P Mark P. Collings, 1 Martin R. S. McCoustra 1 and David A. Williams 2 1 School
More informationPCCP Accepted Manuscript
PCCP Accepted Manuscript This is an Accepted Manuscript, which has been through the Royal Society of Chemistry peer review process and has been accepted for publication. Accepted Manuscripts are published
More informationA Far-ultraviolet Fluorescent Molecular Hydrogen Emission Map of the Milky Way Galaxy
A Far-ultraviolet Fluorescent Molecular Hydrogen Emission Map of the Milky Way Galaxy (The Astrophysical Journal Supplement Series, 231:21 (16pp), 2017 August) November 14, 2017 Young-Soo Jo Young-Soo
More informationProduction of complex organic molecules: H-atom addition versus UV irradiation
MNRAS 467, 25522565 (2017) Advance Access publication 2017 January 25 doi:10.1093/mnras/stx222 Production of complex organic molecules: H-atom addition versus UV irradiation K.-J. Chuang, 1,2 G. Fedoseev,
More informationCryochemistry in the inert and interstellar media
Cryochemistry in the inert and interstellar media Serge A. Krasnokutski Friedrich Schiller University of Jena, 07740 Jena, Germany MPI for Astronomy, Königstuhl 17,69117 Heidelberg, Germany Holes in heaven
More informationH 2 O and CO Ices in Protostellar Environments Recent Keck Telescope Results. Adwin Boogert California Inst. of Technology. Interstellar Ices-I
Interstellar Ices-1 H 2 O and CO Ices in Protostellar Environments Recent Keck Telescope Results Adwin Boogert California Inst. of Technology Jan/2005 Interstellar Ices-I Contents Infrared spectra of highly
More informationInteraction between Single-walled Carbon Nanotubes and Water Molecules
Workshop on Molecular Thermal Engineering Univ. of Tokyo 2013. 07. 05 Interaction between Single-walled Carbon Nanotubes and Water Molecules Shohei Chiashi Dept. of Mech. Eng., The Univ. of Tokyo, Japan
More informationFunctionalized Carbon Nanotubes a key to nanotechnology?
1 27th Max Born Symposium Multiscale Modeling of Real Materials Wroclaw, Sep 19, 2010 Functionalized Carbon Nanotubes a key to nanotechnology? Karolina Milowska, Magda Birowska & Jacek A. Majewski Faculty
More informationPhysical Chemistry Chemical Physics
Physical Chemistry Chemical Physics www.rsc.org/pccp Volume 13 Number 23 21 June 2011 Pages 10825 11452 ISSN 1463-9076 COVER ARTICLE Head et al. A computational study on the structures of methylamine carbon
More informationDesign of Efficient Catalysts with Double Transition Metal. Atoms on C 2 N Layer
Supporting Information Design of Efficient Catalysts with Double Transition Metal Atoms on C 2 N Layer Xiyu Li, 1, Wenhui Zhong, 2, Peng Cui, 1 Jun Li, 1 Jun Jiang 1, * 1 Hefei National Laboratory for
More informationDust in the Diffuse Universe
Dust in the Diffuse Universe Obscuring Effects Chemical Effects Thermal Effects Dynamical Effects Diagnostic Power Evidence for Grains: Chemical Effects Catalyzes molecular hydrogen formation. Depletion
More informationExperimental and Quantum Investigation on Ice Surface Structure and Reactivity
Experimental and Quantum Investigation on Ice Surface Structure and Reactivity A.Allouche J.P.Aycard F.Borget T.Chiavassa I.Couturier C.Manca F.Marinelli C.Martin S.Raunier P.Roubin Physique des Interactions
More informationElectronic Supplementary Information
Electronic Supplementary Material (ESI) for Green Chemistry. This journal is The Royal Society of Chemistry 2016 Electronic Supplementary Information Interfacial acidity in ligand-modified ruthenium nanoparticles
More informationNovel astrochemical aspects of cyanoacetylene-related molecules
Novel astrochemical aspects of cyanoacetylene-related molecules R. KOŁOS 1,2, M. GRONOWSKI 1 & M. TUROWSKI 1 1) Institute of Physical Chemistry, Polish Academy of Sciences, Warsaw 2) Faculty of Mathematics
More informationInterstellar Dust and Extinction
University of Oxford, Astrophysics November 12, 2007 Outline Extinction Spectral Features Emission Scattering Polarization Grain Models & Evolution Conclusions What and Why? Dust covers a range of compound
More informationMechanisms of H- and OH-assisted CO activation as well as C-C coupling on the flat Co(0001) surface Revisited
Electronic Supplementary Material (ESI) for Catalysis Science & Technology. This journal is The Royal Society of Chemistry 2016 Mechanisms of H- and OH-assisted CO activation as well as C-C coupling on
More informationHigh Resolution Spectroscopy and Astronomical Detection of Molecular Anions
High Resolution Spectroscopy and Astronomical Detection of Molecular Anions Sandra Brünken, C. A. Gottlieb, H. Gupta, M. C. McCarthy, and P.Thaddeus Harvard Smithsonian Center for Astrophysics 10th Biennial
More informationBroadband Nitrile Reaction Screening. Kiera Matthews Hanifah Hendricks
Broadband Nitrile Reaction Screening Kiera Matthews Hanifah Hendricks Acknowledgements Brooks Pate - University of Virginia Justin Neill University of Virginia Sarah Payne - University of Virginia Michael
More informationSolid-state formation of complex molecules under dense cloud conditions
Solid-state formation of complex molecules under dense cloud conditions Gleb Fedoseev 1,2 K.-J. Chuang 2,3, S. Ioppolo 4, E. F. van Dishoeck 3, M. E. Palumbo 1 and H. Linnartz 2 1 INAF Osservatorio Astrofisico
More informationSupplementary Figure 1 Morpholigical properties of TiO 2-x SCs. The statistical particle size distribution (a) of the defective {001}-TiO 2-x SCs and
Supplementary Figure 1 Morpholigical properties of TiO 2-x s. The statistical particle size distribution (a) of the defective {1}-TiO 2-x s and their typical TEM images (b, c). Quantity Adsorbed (cm 3
More information