The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

The time-scales for galaxy quenching offer clues to its underlying physical drivers. We
investigate central galaxy quenching time-scales in the IllustrisTNG 100-1 simulation, their …

We use the eagle simulations to study the connection between the quenching time-scale,
τQ, and the physical mechanisms that transform star-forming galaxies into passive galaxies …

The connection between quenching mechanisms, which rapidly turn star-forming systems
into quiescent, and the properties of the galaxy population remains difficult to discern. In this …

It has been suggested that the bulge-to-total stellar mass ratio or feedback from black holes
(BHs), traced by the BH-to-(total stellar) mass ratio, might establish a galaxy's specific star …

We study recent changes on the star-formation history (SFH) of galaxies by means of the
ageing diagram (AD), tracing the fraction of stars formed during the last∼ 20 Myr through the …

SQuIGG E Survey: Massive z ∼ 0.6 Post-starburst Galaxies Exhibit Flat Age Gradients -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

The distribution of galaxies on a colour–magnitude diagram reveals a bimodality, featuring a
passively evolving red sequence and a star-forming blue cloud. The region between these …

The green valley (GV) represents an important transitional state from actively star-forming
galaxies to passively evolving systems. Its traditional definition, based on colour, rests on a …

We test cosmological hydrodynamical simulations of galaxy formation regarding the
properties of the blue cloud (BC), green valley (GV), and red sequence (RS), as measured …