Galaxies and Supermassive Black Holes

Similar documents
11/8/18. Tour of Galaxies. Our Schedule

View of the Galaxy from within. Lecture 12: Galaxies. Comparison to an external disk galaxy. Where do we lie in our Galaxy?

ASTRO504 Extragalactic Astronomy. 2. Classification

Lecture Outlines. Chapter 24. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Star systems like our Milky Way. Galaxies

Chapter 19 Galaxies. Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past. halo

4/6/17. SEMI-WARM stuff: dust. Tour of Galaxies. Our Schedule

The Galaxy. (The Milky Way Galaxy)

Part two of a year-long introduction to astrophysics:

Lecture Two: Galaxy Morphology:

Chapter 30. Galaxies and the Universe. Chapter 30:

Galaxies. With a touch of cosmology

Chapter 15 The Milky Way Galaxy. The Milky Way

Chapter 15 2/19/2014. Lecture Outline Hubble s Galaxy Classification. Normal and Active Galaxies Hubble s Galaxy Classification

It is about 100,000 ly across, 2,000 ly thick, and our solar system is located 26,000 ly away from the center of the galaxy.

Lecture 19: Galaxies. Astronomy 111

Galaxies. Hubble's measurement of distance to M31 Normal versus other galaxies Classification of galaxies Ellipticals Spirals Scaling relations

24.1 Hubble s Galaxy Classification

An Introduction to Galaxies and Cosmology. Jun 29, 2005 Chap.2.1~2.3

The Milky Way Galaxy

Tour of Galaxies. Sgr A* VLT in IR + adaptive optics. orbits. ASTR 1040 Accel Astro: Stars & Galaxies VLT IR+AO

2 Galaxy morphology and classification

Quasars and Active Galactic Nuclei (AGN)

The Classification of Galaxies

Galaxies. Galaxy Diversity. Galaxies, AGN and Quasars. Physics 113 Goderya

The physical properties of galaxies in Universe

Galaxy Morphology. - a description of the structure of galaxies

Active Galaxies & Quasars

Hubble sequence galaxy classification scheme, originally based on appearance, but correlates with other properties as well.

The Milky Way Galaxy. Some thoughts. How big is it? What does it look like? How did it end up this way? What is it made up of?

midterm exam thurs june 14 morning? evening? fri june 15 morning? evening? sat june 16 morning? afternoon? sun june 17 morning? afternoon?

Galaxies with Active Nuclei. Active Galactic Nuclei Seyfert Galaxies Radio Galaxies Quasars Supermassive Black Holes

Astr 5465 Feb. 13, 2018 Distribution & Classification of Galaxies Distribution of Galaxies

Ay162, Spring 2006 Week 8 p. 1 of 15

Galaxies. Early Attempts to catalog and classify. Messier Catalog. "The Great Debate" PHY galaxies - J. Hedberg

The Universe o. Galaxies. The Universe of. Galaxies. Ajit Kembhavi IUCAA

The Neighbors Looking outward from the Sun s location in the Milky Way, we can see a variety of other galaxies:

Chapter 23 The Milky Way Galaxy Pearson Education, Inc.

Ch. 25 In-Class Notes: Beyond Our Solar System

Chapter 15 The Milky Way Galaxy

Galaxies Guiding Questions

Galaxies. Early Attempts to catalog and classify. Messier Catalog. "The Great Debate"

Galaxies -- Introduction. Classification -- Feb 13, 2014

BHS Astronomy: Galaxy Classification and Evolution

Tour of Galaxies. stuff: dust SEMI-WARM. ASTR 1040 Accel Astro: Stars & Galaxies. Dust+dark molecular clouds. in close-up VLT.

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015

Galaxies. What is a Galaxy? A bit of History. A bit of History. Three major components: 1. A thin disk consisting of young and intermediate age stars

Galaxy classification

ASTR 1120 General Astronomy: Stars & Galaxies

Laboratory: Milky Way

2. Can observe radio waves from the nucleus see a strong radio source there Sagittarius A* or Sgr A*.

Lecture #21: Plan. Normal Galaxies. Classification Properties Distances

ASTR 1120 General Astronomy: Stars & Galaxies

Lecture 30. The Galactic Center

Galaxies: The Nature of Galaxies

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.

Galaxies. Lecture Topics. Lecture 23. Discovering Galaxies. Galaxy properties. Local Group. History Cepheid variable stars. Classifying galaxies

5 Dark matter and dark energy, the Universe revealed

GALAXIES. I. Morphologies and classification 2. Successes of Hubble scheme 3. Problems with Hubble scheme 4. Galaxies in other wavelengths

The Milky Way & Galaxies

Galaxies & Introduction to Cosmology

Figure 1: (Image Credit)

Galaxies. Need a (physically) meaningful way of describing the relevant properties of a galaxy.

Figure 19.19: HST photo called Hubble Deep Field.

Star Formation and U/HLXs in the Cartwheel Galaxy Paper & Pencil Version

Outline. The Rotation of the Galaxy. Astronomy: The Big Picture

Module 3: Astronomy The Universe Topic 2 Content: The Milky Way Galaxy Presentation Notes

4/18/17. Our Schedule. Revisit Quasar 3C273. Dark Matter in the Universe. ASTR 1040: Stars & Galaxies

Active Galactic Nuclei (AGNs): A type of AGNs: Quasars. Whatever is powering these QSO s must be very small!!

Black Holes in Hibernation

Chapter 21 Galaxy Evolution. How do we observe the life histories of galaxies?

Galaxies. CESAR s Booklet

Lecture Outlines. Chapter 23. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Galaxies Galaxy Classification Formation of Galaxies Galactic Evolution

The Milky Way. Mass of the Galaxy, Part 2. Mass of the Galaxy, Part 1. Phys1403 Stars and Galaxies Instructor: Dr. Goderya

Neutron Stars. Neutron Stars and Black Holes. The Crab Pulsar. Discovery of Pulsars. The Crab Pulsar. Light curves of the Crab Pulsar.

M31 - Andromeda Galaxy M110 M32

LESSON 1. Solar System

Arvind Borde / AST 10, Week 2: Our Home: The Milky Way

Physics HW Set 3 Spring 2015

What is the solar system?

Clicker Question: Galaxy Classification. What type of galaxy do we live in? The Variety of Galaxy Morphologies Another barred galaxy

Summary: Nuclear burning in stars

Our Galaxy. Milky Way Galaxy = Sun + ~100 billion other stars + gas and dust. Held together by gravity! The Milky Way with the Naked Eye

Chapter 17. Active Galaxies and Supermassive Black Holes

Active Galactic Nuclei

April 11, Astronomy Notes Chapter 16.notebook. Types of Galaxies

Chapter 15 Galaxies and the Foundation of Modern Cosmology

ASTRONOMY. MINNESOTA REGIONS 2011 by Michael Huberty

Powering the Universe with Supermassive Black Holes. Steve Ehlert and Paul Simeon

Galaxy Classification

29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A

Lecture 9. Quasars, Active Galaxies and AGN

Major Review: A very dense article" Dawes Review 4: Spiral Structures in Disc Galaxies; C. Dobbs and J Baba arxiv "

Stars, Galaxies & the Universe Lecture Outline

STRUCTURE AND DYNAMICS OF GALAXIES

Astr 2320 Thurs. April 27, 2017 Today s Topics. Chapter 21: Active Galaxies and Quasars

A100H Exploring the Universe: Discovering Galaxies. Martin D. Weinberg UMass Astronomy

Lecture 27 Galaxy Types and the Distance Ladder December 3, 2018

THE UNIVERSE CHAPTER 20

Transcription:

Galaxies and Supermassive Black Holes Josh Webster 4/21/2014 4/21/2014 Josh Webster 1 http://www.nasa.gov/images/content/690958main_p1237a1.jpg

A Look Ahead 4/21/2014 Josh Webster 2

A Look Ahead Galaxy Classification Hubble Sequence De Vaucoulers System 4/21/2014 Josh Webster 2

A Look Ahead Galaxy Classification Hubble Sequence De Vaucoulers System Examples of Galaxy Types 4/21/2014 Josh Webster 2

A Look Ahead Galaxy Classification Hubble Sequence De Vaucoulers System Examples of Galaxy Types Active Galactic Nuclei Supermassive Black Holes The center of the Milky Way Gas cloud approaches SGR A* 4/21/2014 Josh Webster 2

Galaxy Classification The Hubble Sequence (1936) http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 6

Galaxy Classification The Hubble Sequence (1936) E featureless ovals, ranging from circular to flattened http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 6

Galaxy Classification The Hubble Sequence (1936) E featureless ovals, ranging from circular to flattened S0 lenticular galaxies w/o spiral structure http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 6

Galaxy Classification The Hubble Sequence (1936) E featureless ovals, ranging from circular to flattened S0 lenticular galaxies w/o spiral structure S[a-c]- tight spiral structure, bright central bulge http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 6

Galaxy Classification The Hubble Sequence (1936) E featureless ovals, ranging from circular to flattened S0 lenticular galaxies w/o spiral structure S[a-c]- tight spiral structure, bright central bulge SB[a-c] same as S[a-c], but has central bar http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 6

Galaxy Classification Continued The De Vaucoulers System (1959) 4/21/2014 Josh Webster 12

Galaxy Classification Continued 4 Main Types: Ellipticals: E Lenticulars: S0 Spirals: S Irregulars: I The De Vaucoulers System (1959) 4/21/2014 Josh Webster 12

Galaxy Classification Continued 4 Main Types: Ellipticals: E Lenticulars: S0 Spirals: S Irregulars: I 4 main stages: From early to late (a, b, c, d) Can also be intermediate (ab, bc, cd) Lenticulars (S0 -, S0 0, S0 + ) E + for late E transitioning to S0 The De Vaucoulers System (1959) 4/21/2014 Josh Webster 12

Galaxy Classification Continued 4 Main Types: Ellipticals: E Lenticulars: S0 Spirals: S Irregulars: I 4 main stages: From early to late (a, b, c, d) Can also be intermediate (ab, bc, cd) Lenticulars (S0 -, S0 0, S0 + ) E + for late E transitioning to S0 The De Vaucoulers System (1959) Irregulars Usually denoted Im Magellanic (m) Transition or spiral type (Sm) Non-magellanic w/ structure related to S0 (I0) 4/21/2014 Josh Webster 12

Galaxy Classification Continued The De Vaucoulers System (1959) 4 Main Types: Ellipticals: E Lenticulars: S0 Spirals: S Irregulars: I Spirals and lenticulars have 2 families: True nonbarred (SA, SA0) True barred (SB, SB0) Intermediate barred (SAB, SAB0) 4 main stages: From early to late (a, b, c, d) Can also be intermediate (ab, bc, cd) Lenticulars (S0 -, S0 0, S0 + ) E + for late E transitioning to S0 Irregulars Usually denoted Im Magellanic (m) Transition or spiral type (Sm) Non-magellanic w/ structure related to S0 (I0) 4/21/2014 Josh Webster 12

Galaxy Classification Continued 4 Main Types: Ellipticals: E Lenticulars: S0 Spirals: S Irregulars: I 4 main stages: From early to late (a, b, c, d) Can also be intermediate (ab, bc, cd) Lenticulars (S0 -, S0 0, S0 + ) E + for late E transitioning to S0 The De Vaucoulers System (1959) Irregulars Usually denoted Im Magellanic (m) Transition or spiral type (Sm) Non-magellanic w/ structure related to S0 (I0) Spirals and lenticulars have 2 families: True nonbarred (SA, SA0) True barred (SB, SB0) Intermediate barred (SAB, SAB0) Spirals and lenticulars have 2 varieties: Ringed (r) Pure spiral (s) Transition (rs) Complete outer ring structure (R) Psuedo-ring from spiral arms, such as in S(s) type, (R ) 4/21/2014 Josh Webster 12

Rings http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 17

An Example of Spiral Varieties True Spiral Transition Ringed True Nonbarred (SA) Intermediate (SAB) True Barred (SB) http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 18

Galaxy Classification Continued http://upload.wikimedia.org/wikipedia/commons/8/85/galaxy_morphology.jpg 4/21/2014 Josh Webster 19

A Closer Look at Galaxies 4/21/2014 Josh Webster 20

Elliptical Galaxies M87 4/21/2014 Josh Webster 26 http://apod.nasa.gov/apod/image/1005/m87jet_block.jpg

Elliptical Galaxies M87 Galaxy type: E1 pec E1: elliptical Pec: peculiar 4/21/2014 Josh Webster 26 http://apod.nasa.gov/apod/image/1005/m87jet_block.jpg

Lenticular Galaxies NGC 524 4/21/2014 Josh Webster 28 http://www.nasa.gov/sites/default/files/potw1329a.jpg

Lenticular Galaxies NGC 524 Galaxy Type: S0 D S0: lenticular type D: rotationally symmetric w/o pronounced spiral 4/21/2014 Josh Webster 28 http://www.nasa.gov/sites/default/files/potw1329a.jpg

M51 Spiral Galaxies NGC 5195 4/21/2014 Josh Webster 30 http://apod.nasa.gov/apod/image/1006/m51_peris.jpg

M51 Spiral Galaxies NGC 5195 Galaxy Type: SA(s)bc pec SA: spiral w/o bars (s): w/o rings bc: intermediate stage Pec: peculiar 4/21/2014 Josh Webster 30 http://apod.nasa.gov/apod/image/1006/m51_peris.jpg

M51 Spiral Galaxies NGC 5195 Galaxy Type: SA(s)bc pec SA: spiral w/o bars (s): w/o rings bc: intermediate stage Pec: peculiar HII region 4/21/2014 Josh Webster 30 http://apod.nasa.gov/apod/image/1006/m51_peris.jpg

4/21/2014 Josh Webster 33 http://upload.wikimedia.org/wikipedia/commons/5/52/hubble2005-01-barred-spiral-galaxy-ngc1300.jpg Barred Spiral Galaxies NGC 1300

Barred Spiral Galaxies NGC 1300 Galaxy Type: SB(rs)bc SB: barred spiral (rs): transition bc: intermediate stage 4/21/2014 Josh Webster 33 http://upload.wikimedia.org/wikipedia/commons/5/52/hubble2005-01-barred-spiral-galaxy-ngc1300.jpg

4/21/2014 Josh Webster 35 http://apod.nasa.gov/apod/image/1102/ngc4449_hlagendlerl.jpg Irregular Galaxies NGC 4449

Irregular Galaxies Galaxy Type: IBm I: Irregular B: Barred m: magellanic NGC 4449 4/21/2014 Josh Webster 35 http://apod.nasa.gov/apod/image/1102/ngc4449_hlagendlerl.jpg

What s at the center of a galaxy? 4/21/2014 Josh Webster 33

What s at the center of a galaxy? 4/21/2014 Josh Webster 33

What s at the center of a galaxy? From what we observe, it appears nearly every galaxy contains a supermassive black hole at its center, and it can be active or inactive. 4/21/2014 Josh Webster 33

Active Galactic Nuclei (AGN) 4/21/2014 Josh Webster 38

Active Galactic Nuclei (AGN) An active core of a galaxy Emits radiation 4/21/2014 Josh Webster 38

Active Galactic Nuclei (AGN) An active core of a galaxy Emits radiation Very high luminosity over a large range of EM spectrum, based on type. 4/21/2014 Josh Webster 38

Active Galactic Nuclei (AGN) An active core of a galaxy Emits radiation Very high luminosity over a large range of EM spectrum, based on type. Radiation believed to be originating from supermassive black hole at center accreting mass. 4/21/2014 Josh Webster 38

Galactic Nuclei Types http://en.wikipedia.org/wiki/active_galactic_nucleus#summary 4/21/2014 Josh Webster 39

Supermassive Black Holes M87 4/21/2014 Josh Webster 40 http://apod.nasa.gov/apod/image/1005/m87jet_block.jpg

Supermassive Black Holes 4/21/2014 Josh Webster 41

Supermassive Black Holes 4/21/2014 Josh Webster 45 http://hubblesite.org/newscenter/archive/releases/2000/20/image/a/

4/21/2014 Josh Webster 45 http://hubblesite.org/newscenter/archive/releases/2000/20/image/a/ Supermassive Black Holes Jet of emitted sub-atomic particles from a source of mass 2 billion times that of the sun.

4/21/2014 Josh Webster 45 http://hubblesite.org/newscenter/archive/releases/2000/20/image/a/ Supermassive Black Holes Jet of emitted sub-atomic particles from a source of mass 2 billion times that of the sun.

Center of the Milky Way 4/21/2014 Josh Webster 45 http://upload.wikimedia.org/wikipedia/commons/4/43/eso-vlt-laser-phot-33a-07.jpg

Center of the Milky Way Chandra X-Ray Observatory SGR A* using VLA (radio) https://www.e-education.psu.edu/astro801/content/l8_p7.html 4/21/2014 Josh Webster 46

T 10 8 K 2 day period Center of the Milky Way: SGR A* NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

T 10 8 K 2 day period Center of the Milky Way: SGR A* Black hole at the center: NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

T 10 8 K 2 day period Center of the Milky Way: SGR A* Black hole at the center: 4 million times the mass of the sun NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

T 10 8 K 2 day period Center of the Milky Way: SGR A* Black hole at the center: 4 million times the mass of the sun 26,000 Ly from Earth NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

T 10 8 K 2 day period Center of the Milky Way: SGR A* Black hole at the center: 4 million times the mass of the sun 26,000 Ly from Earth Faint X-ray emission NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

T 10 8 K 2 day period Center of the Milky Way: SGR A* Black hole at the center: 4 million times the mass of the sun 26,000 Ly from Earth Faint X-ray emission Only 1% of material in vicinity reaches event horizon NuSTAR http://en.wikipedia.org/wiki/file:pointing_x-ray_eyes_at_our_resident_supermassive_black_hole.jpg 4/21/2014 Josh Webster 51

Stellar Orbits Near SGR A* S2 orbit 15.24 years Sedna 11,400 years S2 velocity 5000 km/s 1.67% speed of light That s 166x Earth s orbit speed! http://en.wikipedia.org/wiki/file:galactic_centre_orbits.svg 4/21/2014 Josh Webster 53

4/21/2014 Josh Webster 54 http://en.wikipedia.org/wiki/file:g2cloud_eso1151a.jpeg Gas Cloud (G2) Near SGR A* Cloud roughly 10 times the mass of Earth

Conclusion 4/21/2014 Josh Webster 55

Conclusion Classifying galaxies and their evolution stages proved to be quite difficult. 4/21/2014 Josh Webster 55

Conclusion Classifying galaxies and their evolution stages proved to be quite difficult. There are many varieties of galaxies. Their classification can give an idea of what stage of evolution they are in. 4/21/2014 Josh Webster 55

Conclusion Classifying galaxies and their evolution stages proved to be quite difficult. There are many varieties of galaxies. Their classification can give an idea of what stage of evolution they are in. The De Vaucoulers system is an extension of the Hubble sequence, and is the most commonly used. 4/21/2014 Josh Webster 55

Conclusion Classifying galaxies and their evolution stages proved to be quite difficult. There are many varieties of galaxies. Their classification can give an idea of what stage of evolution they are in. The De Vaucoulers system is an extension of the Hubble sequence, and is the most commonly used. Astrophysics is a rapidly developing field of science. There is still much that we don t understand about galaxies. The technology to observe certain phenomena has only recently become available. Everything prior to the early-mid 1900 s was theory or just speculation. 4/21/2014 Josh Webster 55

References De Vaucoulers, G. (1962). Revised Classification of 1500 Bright Galaxies. Accessed April 18, 2014 from: http://articles.adsabs.harvard.edu/cgi-bin/nphiarticle_query?1963apjs...8...31d&data_type=pdf_high&whole_paper =YES&type=PRINTER&filetype=.pdf Ciardullo, R. (2009). Galaxy Classification. Accessed April 18, 2014 from: http://www2.astro.psu.edu/users/rbc/a504/classifications.pdf Torres, Diego F. & Anchordoqui, Luis A. (2004). Astrophysical Origins of Ultrahigh Energy Cosmic Rays. Accessed April 18, 2014 from: http://ned.ipac.caltech.edu/level5/march04/torres/torres_contents.html NASA & The Hubble Heritage Team (2000). A Cosmic Searchlight. Accessed April 18, 2014 from: http://hubblesite.org/newscenter/archive/releases/2000/20/image/a/ Boen, Brooke. (2013). Supermassive Black Hole Sagittarius A*. Accessed April 18, 2014 from: http://www.nasa.gov/mission_pages/chandra/multimedia/black-hole- SagittariusA.html Murdin, P. & Buta, Ronald (2006). Encyclodpedia of Astronomy and Astrophysics. Accessed April 18, 2014 from: http://www.astro.caltech.edu/~george/ay21/eaa/eaa-classif.pdf 4/21/2014 Josh Webster 60

Questions? 4/21/2014 Josh Webster 61