Star-forming galaxies at cosmic noon

NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

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 …

Introducing the NEWHORIZON simulation: Galaxy properties with resolved internal dynamics across cosmic time

Y Dubois, R Beckmann, F Bournaud, H Choi… - Astronomy & …, 2021 - aanda.org
Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics …

Physical models of galaxy formation in a cosmological framework

RS Somerville, R Davé - Annual Review of Astronomy and …, 2015 - annualreviews.org
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 …

The evolution of galaxy structure over cosmic time

CJ Conselice - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

The SINFONI black hole survey: the black hole fundamental plane revisited and the paths of (co) evolution of supermassive black holes and bulges

RP Saglia, M Opitsch, P Erwin, J Thomas… - The Astrophysical …, 2016 - iopscience.iop.org
We investigate the correlations between the black hole (BH) mass M BH, the velocity
dispersion σ, the bulge mass M Bu, the bulge average spherical density ${\rho} _ {{\rm {h}}} …

The SINS/zC-SINF Survey of z∼ 2 Galaxy Kinematics: SINFONI Adaptive Optics–assisted Data and Kiloparsec-scale Emission-line Properties∗

NMF Schreiber, A Renzini, C Mancini… - The Astrophysical …, 2018 - iopscience.iop.org
We present the" SINS/zC-SINF AO survey" of 35 star-forming galaxies, the largest sample
with deep adaptive optics (AO)–assisted near-infrared integral field spectroscopy at z∼ 2 …

The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function

MR Krumholz - Physics Reports, 2014 - Elsevier
Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

Kiloparsec-scale dust disks in high-redshift luminous submillimeter galaxies

JA Hodge, AM Swinbank, JM Simpson… - The Astrophysical …, 2016 - iopscience.iop.org
We present high-resolution (0 farcs 16) 870 μm Atacama Large Millimeter/submillimeter
Array (ALMA) imaging of 16 luminous (${L} _ {\mathrm {IR}}\sim 4\times {10}^{12}\,{L} …

Observational constraints on the feeding of supermassive black holes

T Storchi-Bergmann, A Schnorr-Müller - Nature Astronomy, 2019 - nature.com
Supermassive black holes grow at the centre of galaxies in consonance with them. In this
Review Article, we discuss the mass-feeding mechanisms that lead to this growth in active …