Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

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 …

We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …

We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …

Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and
Quiescent Galaxies - IOPscience This site uses cookies. By continuing to use this site you …

Using the IllustrisTNG simulations, we investigate the connection between galaxy
morphology and star formation in central galaxies with stellar masses in the range 109 …

We present Hα maps at 1 kpc spatial resolution for star-forming galaxies at z∼ 1, made
possible by the Wide Field Camera 3 grism on Hubble Space Telescope (HST). Employing …

Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

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 …

Structural Evolution in Massive Galaxies at z ∼ 2 - IOPscience This site uses cookies. By
continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and …