Results 31 to 40 of about 6,393 (178)
Shape asymmetry : a morphological indicator for automatic detection of galaxies in the post-coalescence merger stages [PDF]
MMP and VW acknowledge support from the European Career Reintegration Grant Phiz-Ev (P.I. VW). VW, KR and JM-A acknowledge support from the European Research Council Starting Grant SEDMorph (P.I. VW).
Wild, V. +16 more
core +1 more source
Rise and fall of post-starburst galaxies in Magneticum Pathfinder [PDF]
ABSTRACT Post-starburst (PSB) galaxies belong to a short-lived transition population between star-forming (SF) and quiescent galaxies. Deciphering their heavily discussed evolutionary pathways is paramount to understanding galaxy evolution.
Lotz, M. +3 more
openaire +4 more sources
Five E+A (post-starburst) galaxies as Brightest Cluster Galaxies [PDF]
Brightest Cluster Galaxies (BCGs) are mostly elliptical galaxies and very rarely have prominent star formations. We found that five out of 8,812 BCGs are E+A (i.e., post-starburst) galaxies, having an Hδ absorption line with an equivalent width >2.5 A and no distinct emission lines in [O II] and Hα −.
FengShan Liu +3 more
openaire +1 more source
Fading AGN in Post-Starburst Galaxies
The role of AGN in quenching galaxies and driving the evolution from star-forming to quiescent remains a key question in galaxy evolution. We present evidence from the Mapping Nearby Galaxies at APO (MaNGA) survey for fading AGN activity in 6/93 post ...
Earl, Nicholas +13 more
core +1 more source
Two main physical processes characterize the activity in the nuclear region of active galaxies: an intense star formation (starburst, SB) and an Active Galactic Nucleus (AGN).
Eleonora Sani
doaj +1 more source
After the Fall: The Dust and Gas in E+A Post-starburst Galaxies [PDF]
Abstract 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 a significant interstellar medium (ISM) in many post-starburst galaxies raise important questions.
A. Smercina +13 more
openaire +4 more sources
Star formation and molecular gas properties of post-starburst galaxies
Post-starburst galaxies are believed to be in a rapid transition between major merger starbursts and quiescent ellipticals. Their optical spectrum is dominated by A-type stars, suggesting a starburst that was quenched recently. While optical observations
French, K. +17 more
core +1 more source
On Post-starburst Galaxies Dominating Tidal Disruption Events [PDF]
Abstract A starburst induced by a galaxy merger may create a relatively thin central stellar disk at radius ≤100 pc. We calculate the rate of tidal disruption events (TDEs) by the inspiraling secondary supermassive black hole (SMBH) through the disk. With a small enough stellar velocity dispersion (
openaire +2 more sources
Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
We present the Cosmic Sands suite of cosmological zoom-in simulations based on the simba galaxy formation model in order to study the buildup of the first massive and dusty galaxies in the early universe.
Sidney Lower +3 more
doaj +1 more source
The cold gas content of post-starburst galaxies [PDF]
Post-starburst galaxies, or E+A galaxies, are characterized by optical spectra showing strong Balmer absorption lines, indicating a young stellar population, and little or no emission lines, implying no active star formation. These galaxies are interpreted as a transitional population between star-forming, disc-dominated galaxies and spheroidal ...
Zwaan, Martin A. +3 more
openaire +3 more sources

