The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …

Detailed modeling of the recent star formation histories (SFHs) of post-starburst (or" E+ A")
galaxies is impeded by the degeneracy between the time elapsed since the starburst ended …

Post-starburst galaxies are sources that had the last major episode of star formation about 1
Gyr before the epoch of the observations and are on their way to quiescence. It is important …

Feedback from active galactic nuclei (AGNs) is expected to impact the amount of cold gas in
galaxies by driving strong galactic winds, by preventing external gas inflows, or by changing …

The traditional picture of post-starburst galaxies as dust-and gas-poor merger remnants,
rapidly transitioning to quiescence, has been recently challenged. Unexpected detections of …

ABSTRACT E+ A galaxies are believed to be a short phase connecting major merger
ultraluminous infrared galaxies (ULIRGs) with red and dead elliptical galaxies. Their optical …

Post-starburst E+ A galaxies are systems that hosted a powerful starburst that was quenched
abruptly. Simulations suggest that these systems provide the missing link between major …

Post-starburst (PSB) galaxies have recently and rapidly quenched their star formation; thus,
they are an important way to understand how galaxies transition from star-forming late types …

Dirt-cheap Gas Scaling Relations: Using Dust Absorption, Metallicity, and Galaxy Size to Predict
Gas Masses for Large Samples of Galaxies - IOPscience This site uses cookies. By continuing …

Post-starburst galaxies are typically considered to be a transition population, en route to the
red sequence after a recent quenching event. Despite this, recent observations have shown …