What drives the growth of black holes?
DM Alexander, RC Hickox - New Astronomy Reviews, 2012 - Elsevier
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
Theoretical modeling of starburst galaxies
We have modeled a large sample of infrared starburst galaxies using both the PEGASE v2.
0 and STARBURST99 codes to generate the spectral energy distribution (SED) of the young …
0 and STARBURST99 codes to generate the spectral energy distribution (SED) of the young …
[图书][B] Ultraluminous infrared galaxies
CJ Lonsdale, D Farrah, HE Smith - 2006 - Springer
Ever since their discovery in the 1970's, UltraLuminous InfraRed Galaxies (ULIRGs;
classically L ir> 10 12 L⊙) have fascinated astronomers with their immense luminosities …
classically L ir> 10 12 L⊙) have fascinated astronomers with their immense luminosities …
Fast molecular outflows in luminous galaxy mergers: evidence for quasar feedback from Herschel
S Veilleux, M Meléndez, E Sturm… - The Astrophysical …, 2013 - iopscience.iop.org
We report the results from a systematic search for molecular (OH 119 μm) outflows with
Herschel/PACS in a sample of 43 nearby (z< 0.3) galaxy mergers, mostly ultraluminous …
Herschel/PACS in a sample of 43 nearby (z< 0.3) galaxy mergers, mostly ultraluminous …
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured
Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
The dust opacity of star‐forming galaxies
D Calzetti - Publications of the Astronomical Society of the Pacific, 2001 - iopscience.iop.org
The presence of dust in galaxies removes one‐half or more of the stellar energy from the UV‐
optical budget of the universe and has a profound impact on our understanding of how …
optical budget of the universe and has a profound impact on our understanding of how …
The multiphase structure and power sources of galactic winds in major mergers
DSN Rupke, S Veilleux - The Astrophysical Journal, 2013 - iopscience.iop.org
Massive, galaxy-scale outflows are known to be ubiquitous in major mergers of disk galaxies
in the local universe. In this paper, we explore the multiphase structure and power sources …
in the local universe. In this paper, we explore the multiphase structure and power sources …
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 …
Ionized gas outflows and global kinematics of low-z luminous star-forming galaxies
S Arribas, L Colina, E Bellocchi, R Maiolino… - Astronomy & …, 2014 - aanda.org
We study the kinematic properties of the ionised gas outflows and ambient interstellar
medium (ISM) in a large and representative sample of local luminous and ultra-luminous …
medium (ISM) in a large and representative sample of local luminous and ultra-luminous …
Infrared radiation from an extrasolar planet
D Deming, S Seager, LJ Richardson, J Harrington - Nature, 2005 - nature.com
A class of extrasolar giant planets—the so-called 'hot Jupiters'(ref.)—orbit within 0.05 au of
their primary stars (1 au is the Sun–Earth distance). These planets should be hot and so emit …
their primary stars (1 au is the Sun–Earth distance). These planets should be hot and so emit …