Physical models of galaxy formation in a cosmological framework
Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …
challenges in astrophysics today due to the vast range of scales and numerous physical …
Cool gas in high-redshift galaxies
CL Carilli, F Walter - Annual Review of Astronomy and …, 2013 - annualreviews.org
Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …
The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
The ATLAS3D project is a multiwavelength survey combined with a theoretical modelling
effort. The observations span from the radio to the millimetre and optical, and provide …
effort. The observations span from the radio to the millimetre and optical, and provide …
A cosmological framework for the co-evolution of quasars, supermassive black holes, and elliptical galaxies. I. Galaxy mergers and quasar activity
PF Hopkins, L Hernquist, TJ Cox… - The Astrophysical …, 2008 - iopscience.iop.org
We develop a model for the cosmological role of mergers in the evolution of starbursts,
quasars, and spheroidal galaxies. By combining theoretically well-constrained halo and …
quasars, and spheroidal galaxies. By combining theoretically well-constrained halo and …
A semi-analytic model for the co-evolution of galaxies, black holes and active galactic nuclei
We present a new semi-analytic model that self-consistently traces the growth of
supermassive black holes (BH) and their host galaxies within the context of the Lambda cold …
supermassive black holes (BH) and their host galaxies within the context of the Lambda cold …
Theoretical challenges in galaxy formation
T Naab, JP Ostriker - Annual review of astronomy and …, 2017 - annualreviews.org
Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …
evolution. Over the decades the field has made significant progress. It is now possible to …
Formation of massive galaxies at high redshift: cold streams, clumpy disks, and compact spheroids
We present a simple theoretical framework for massive galaxies at high redshift, where the
main assembly and star formation occurred, and report on the first cosmological simulations …
main assembly and star formation occurred, and report on the first cosmological simulations …
Morphological quenching of star formation: making early-type galaxies red
We point out a natural mechanism for quenching of star formation in early-type galaxies
(ETGs). It automatically links the color of a galaxy with its morphology and does not require …
(ETGs). It automatically links the color of a galaxy with its morphology and does not require …
Structure and kinematics of early-type galaxies from integral field spectroscopy
M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
High-redshift star formation in the Atacama large millimetre/submillimetre array era
JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …