Coevolution (or not) of supermassive black holes and host galaxies
J Kormendy, LC Ho - Annual Review of Astronomy and …, 2013 - annualreviews.org
Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …
Powerful outflows and feedback from active galactic nuclei
A King, K Pounds - Annual Review of Astronomy and …, 2015 - annualreviews.org
Active galactic nuclei (AGNs) represent the growth phases of the supermassive black holes
in the center of almost every galaxy. Powerful, highly ionized winds, with velocities∼ 0.1–0.2 …
in the center of almost every galaxy. Powerful, highly ionized winds, with velocities∼ 0.1–0.2 …
The host galaxies of active galactic nuclei
G Kauffmann, TM Heckman, C Tremonti… - Monthly Notices of …, 2003 - academic.oup.com
We examine the properties of the host galaxies of 22 623 narrow-line active galactic nuclei
(AGN) with 0.02< z< 0.3 selected from a complete sample of 122 808 galaxies from the …
(AGN) with 0.02< z< 0.3 selected from a complete sample of 122 808 galaxies from the …
Quasar feedback revealed by giant molecular outflows
C Feruglio, R Maiolino, E Piconcelli, N Menci… - Astronomy & …, 2010 - aanda.org
In the standard scenario for galaxy evolution young star-forming galaxies transform into red
bulge-dominated spheroids, where star formation has been quenched. To explain this …
bulge-dominated spheroids, where star formation has been quenched. To explain this …
Structure and formation of elliptical and spheroidal galaxies
J Kormendy, DB Fisher, ME Cornell… - The Astrophysical …, 2009 - iopscience.iop.org
New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with
published data to derive composite profiles of brightness, ellipticity, position angle, isophote …
published data to derive composite profiles of brightness, ellipticity, position angle, isophote …
Submillimeter galaxies at z~ 2: evidence for major mergers and constraints on lifetimes, IMF, and CO-H2 conversion factor
LJ Tacconi, R Genzel, I Smail, R Neri… - The Astrophysical …, 2008 - iopscience.iop.org
We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z\sim 2
submillimeter galaxies (SMGs), and sensitive CO (3-2) flux limits toward three z\sim 2 …
submillimeter galaxies (SMGs), and sensitive CO (3-2) flux limits toward three z\sim 2 …
How do disks survive mergers?
PF Hopkins, TJ Cox, JD Younger… - The Astrophysical …, 2009 - iopscience.iop.org
We develop a general physical model for how galactic disks survive and/or are destroyed in
mergers and interactions. Based on simple dynamical arguments, we show that gas …
mergers and interactions. Based on simple dynamical arguments, we show that gas …
Clearing out a galaxy
K Zubovas, A King - The Astrophysical Journal Letters, 2012 - iopscience.iop.org
It is widely suspected that active galactic nucleus (AGN) activity ultimately sweeps galaxies
clear of their gas. We work out the observable properties required to achieve this. Large …
clear of their gas. We work out the observable properties required to achieve this. Large …
Spitzer quasar and ulirg evolution study (quest). IV. Comparison of 1 Jy ultraluminous infrared galaxies with palomar-green quasars
S Veilleux, DSN Rupke, DC Kim… - The Astrophysical …, 2009 - iopscience.iop.org
We report the results from a comprehensive study of 74 ultraluminous infrared galaxies
(ULIRGs) and 34 Palomar-Green (PG) quasars within z∼ 0.3 observed with the Spitzer …
(ULIRGs) and 34 Palomar-Green (PG) quasars within z∼ 0.3 observed with the Spitzer …
Outflows in infrared-luminous starbursts at z< 0.5. II. Analysis and discussion
DS Rupke, S Veilleux, DB Sanders - The Astrophysical Journal …, 2005 - iopscience.iop.org
We have performed an absorption-line survey of outflowing gas in 78 starburst-dominated,
infrared-luminous galaxies. This is the largest study of superwinds at z≲ 3. Superwinds are …
infrared-luminous galaxies. This is the largest study of superwinds at z≲ 3. Superwinds are …