Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
Thales A. Gutcke, Andrea V. Macci\`o, Aaron A. Dutton, Greg S. Stinson

TL;DR
This study shows that massive elliptical galaxies can form through a gradual starvation process without the need for sudden quenching, challenging traditional models of galaxy evolution.
Contribution
It introduces a simple starvation model demonstrating that gradual gas cooling suppression can produce realistic elliptical galaxies by z=0 without abrupt quenching events.
Findings
Galaxies can evolve into ellipticals through slow cooling suppression.
Color transition times are less than 1 Gyr, faster than previously thought.
Gradual starvation suffices to explain observed galaxy properties at z=0.
Abstract
The decrease in star formation (SF) and the morphological change necessary to produce the elliptical galaxy population are commonly ascribed to a sudden quenching event, which is able to rid the central galaxy of its cold gas reservoir in a short time. Following this event, the galaxy is able to prevent further SF and stay quiescent via a maintenance mode. We test whether such a quenching event is truly necessary using a simple model of quiescence. In this model, hot gas (all gas above a temperature threshold) in a halo mass galaxy at redshift is prevented from cooling. The cool gas continues to form stars at a decreasing rate and the galaxy stellar mass, morphology, velocity dispersion and position on the color magnitude diagram (CMD) proceed to evolve. By , the halo mass has grown to and the galaxy has attained…
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