Galaxy Evolution Insights from Spatially & Spectrally Resolved Studies

Transcription

1 Galaxy Evolution Insights from Spatially & Spectrally Resolved Studies N.M. Förster Schreiber and the KMOS 3D, SINS/zC-SINF, 3D-HST, PHIBSS/2 Teams E. Wisnioski, E. Wuyts, S. Wuyts, R. Genzel, L.J. Tacconi, P. Lang, D. Lutz, M. Fossati, D. Wilman, A. Renzini, S. Tacchella, M. Carollo K. Bandara, A. Beifiori, R. Bender, N. Bouché, G. Brammer, A. Burkert, J. Chan, A. Cimatti, G. Cresci, E. Daddi, R. Davies, D. Erb, A. Galametz, S. Kulkarni, S. Lilly, C. Mancini, J.T. Mendel, I. Momcheva, T. Naab, E.J. Nelson, S. Newman, Y. Peng, D. Rosario, R. Saglia, S. Seitz, A. Shapley, C. Steidel, A. Sternberg, E. Strobl-Hicks, K. Tadaki, H. Übler, P. van Dokkum, D. Vergani, G. Zamorani

2 KMOS 24 IFUs SINFONI & AO Physics of Galaxy Evolution from In Situ IFU Studies Mass assembly Star formation Structural buildup Chemical enrichment Feedback Quenching SINS/zC-SINF 110 SFGs at z ~ w/ deep AO follow-up KMOS 3D 600+ M -selected z~ SFGs Deep+wide coverage in M -SFR-UVJ E.g., NMFS+06,09,16; Mancini+11; Wisnioski+15,16; Genzel+06,08,11,14; E.Wuyts+14,16; S. Wuyts+16

3 Rich Morphologies of z~1 3 SFGs IJH HST/CANDELS KMOS 3D Wisnioski+15 E.g., Labbé+03;Lotz+06,08,10; Elmegreen+07-09;Kriek+09;NMFS+11a,b;Guo+12,15;Szomoru+13;Nelson+13;Tacchella+15a,b;Tadaki+14a;Cibinel+15

4 Smoother Stellar Structure of z~1 3 SFGs And e.g. Kauffmann+03,06;Schiminovich+07;Bell+08,12;Cheung+12;Bruce+12,14;Fang+13;Bluck+14 ; Hunter+98;Martig+09,13;Saintonge+12;Crocker+12 M HST/CANDELS (M*) Wuyts+12; Lang+14 Wuyts+13; Nelson+13,15; Genzel+14a; Tacchella+15a.b

5 Majority of Disk Kinematics of z~1 3 SFGs H VFs VLT/KMOS 3D Wisnioski+15 Wisnioski+15; Genzel+06,08,11; NMFS+06,09,15; Shapiro+08; Cresci+09; Tacconi+13; Newman+13 Also, e.g., Law+09,12;Epinat+09-12;Jones+10;Green+10; Wisnioski+11,12; Yuan+11,12;Kassin+12; Sobral+13;Stott+14; Livermore+15; Leethochawalit+15

6 Outer Rotation Curves & Angular Momenta Falling outer rotation curves pressure-driven disk truncation? Specific angular momentum of disks reflects that of their DM halos Stack of ~100 log(m ) > 9.7, 0.8 z 2.6 SFGs 360 log(m ) > 9.3, 0.8 z 2.6 SFGs baryons ~ ~ DM (baryons) ~ (DM) v R v 2 Rd rot circ 0 Burkert+15; Lang+16 in prep. / Also S.Wuyts+16 in prep. NMFS/Genzel+06 11; Wisnioski+15. Also, e.g., Kassin+07,12; Epinat+09,12; Law+09,12; Wright+09; Swinbank+12a,b; Jones+10; Sobral+13; Stott+14 Also, e.g., NFW+97; Mo+98; Bullock+01; Sofue&Rubin01; Hetznecker+06; Courteau+07; Burkert+10; van der Kruit&Freeman11; Barnabè+12; Bovy&Rix13; Moster+13; Dutton+13; Cappellari+13; Dekel&Burkert14; Übler+14; Genel+14; Courteau&Dutton15; and many more

7 Vigorous Outflows Driven by Star Formation SINFONI+AO FWHM ~ 450 km/s, across disks, at/near SF clumps Hα narrow Star formation dm out /dt (ionized gas) ~ 1 5 SFRs Breakout at (SFR) 1 M /yr/kpc 2 B 1.0 ZC clump B Star formation 0.5 Outflow Hα broad Outflow velocity offset (km/s) Stacked pixels 1 (8kpc) Genzel+11; Newman+12a,b; Shapiro+09 Also, Pettini+00; Heckman+03,15; Shapley+03;Weiner+09; Steidel+10; Coil+11; Kulas+11; Law+12b; Kornei+12; Chen+12; Martin+05; Rupke+02 13; Sharp,Bland-Hawthorn10; Sturm+11; Westmoquette+12,13; Bouché+12,14; RodríguezZaurín+13; Cicone+14; and many others

8 Ubiquitous Nuclear Outflows Driven by AGN Centers of log(m * ) 10.9 galaxies, FWHM ~ km/s, in H +[NII]+[SII], 2 3 kpc extent High duty cycle among typical massive galaxies, dm out /dt (ionized gas) ~ SFR, v out > v esc D3a-6004 (z=2.38) SINFONI+AO NMFS+14; Genzel+14b; + in prep. Hα broad (outflow) Hα narrow (star formation) Rest-V continuum (stars,hst) 320 M -selected 0.8 z 2.6 galaxies; 80 at log(m ) > 10.8 (KMOS 3D, SINS/zC-SINF, LUCI, GNIRS).Also, e.g., Rupke+02-13; Sturm+11; Nesvadba+11; Westmoquette+12,13; Harrison+12,14; Maiolino+12; Cano Diaz+12; Fabian12; Diamond-Stanic+12; Mullaney+13; Rodriguez-Zaurin+13; Cicone+12,14,15; Juneau+12,14; Brusa+15; Cresci+15; Perna+15

9 Ubiquitous Nuclear Outflows Driven by AGN Centers of log(m * ) 10.9 galaxies, FWHM ~ km/s, in H +[NII]+[SII], 2 3 kpc extent High duty cycle among typical massive galaxies, dm out /dt (ionized gas) ~ SFR, v out > v esc D3a-6004 (z=2.38) SINFONI+AO NMFS+14; Genzel+14b; + in prep. Hα broad (outflow) Hα narrow (star formation) Rest-V continuum (stars,hst) 320 M -selected 0.8 z 2.6 galaxies; 80 at log(m ) > 10.8 (KMOS 3D, SINS/zC-SINF, LUCI, GNIRS).Also, e.g., Rupke+02-13; Sturm+11; Nesvadba+11; Westmoquette+12,13; Harrison+12,14; Maiolino+12; Cano Diaz+12; Fabian12; Diamond-Stanic+12; Mullaney+13; Rodriguez-Zaurin+13; Cicone+12,14,15; Juneau+12,14; Brusa+15; Cresci+15; Perna+15

10 The Need for Sensitive Spatially-Resolved Data K20-ID7 z = 2.2 KMOS (noao) IJH HST h SINFONI+AO M = M SFR = 210 M / yr F(Ha) = cgs R e (H, M ) 8 kpc n (H, M ) 0.2 NMFS+09,15; Tacchella+15a; Lang+14

11 The Need for Sensitive Spatially-Resolved Data D3a15504 z = 2.4 H Corrected for VF Not corrected for VF SINFONI+AO V (H ) SINFONI+AO M HST/WFC3 M = M SFR = 150 M / yr F(Ha) = cgs FWFMbroad (nucl.) = 1000 km/s Fbroad/Ftotal (nucl.) = 0.7 Genzel+06,14; NMFS+14

12 Outlook Physics of lifecycle of massive galaxies from resolved in-situ studies Cold gas/dust on par with Opt/NIR Mass Accretion Star formation Outflows Cold molecular gas Structural buildup Quenching PdBI/NOEMA Tacconi+10,13 NOEMA ALMA

13 Towards Resolving Distant Galaxies on 100pc Scales z = 2.0 D = 4.5 Mpc ( 20 L) Deep near-ir imaging M83 log(m * ) ~ 10.6 SFR ~ 4 M /yr f gas ~ 10-15% 5 kpc kpc resolution HST/WFC3 JWST/NIRCAM E-ELT/MICADO VLT+AO 1.5 ~ 35 pc resolution Larsen+99 Sims details: Trippe et al. (2010) Mock z=2.3 galaxy, EELT resolution ~100 pc Compact clusters detected to K AB ~ 28.5 (M R,AB ~ 16)