Results 31 to 40 of about 4,901,298 (173)

Star formation and molecular gas properties of post-starburst galaxies [PDF]

, 2023
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., Netzer, Hagai, Dieter Lutz, Davies, R., Lutz, Dieter, Prochaska, J. Xavier, Dalya Baron, French, K. Decker, Hagai Netzer, Richard I Davies, J Xavier Prochaska, K Decker French, Netzer, H., Davies, Ric I., Baron, D., Prochaska, J., Lutz, D., Baron, Dalya   +17 more
core   +1 more source

The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample [PDF]

, 2022
We present structural measurements of 145 spectroscopically selected intermediate-redshift (z ∼ 0.7), massive (M⋆ ∼ 1011 M⊙) post-starburst galaxies from the $\mathrm{SQuIGG}\vec{L}{\rm{E}}$ sample measured using wide-depth Hyper Suprime-Cam i-band ...
Spilker, Justin S; https://orcid.org/, Suess, Katherine A; https://orcid.org/, Narayanan, Desika; https://orcid.org/, Kado-Fong, Erin; https://orcid.org/, Hall-Hooper, Khalil, Verrico, Margaret; https://orcid.org/, Setton, David J; https://orcid.org/, Greene, Jenny E; https://orcid.org/, Kriek, Mariska; https://orcid.org/, Bezanson, Rachel; https://orcid.org/, Feldmann, Robert; https://orcid.org/, Goulding, Andy D; https://orcid.org/   +11 more
core   +1 more source

Five E+A (post-starburst) galaxies as Brightest Cluster Galaxies [PDF]

Science China Physics, Mechanics and Astronomy, 2012
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, ZhongLue Wen, JinLin Han, XianMin Meng   +3 more
openaire   +1 more source

Rise and fall of post-starburst galaxies in Magneticum Pathfinder [PDF]

Monthly Notices of the Royal Astronomical Society, 2021
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., Dolag, K., Remus, R., Burkert, A.   +3 more
openaire   +4 more sources

On Post-starburst Galaxies Dominating Tidal Disruption Events [PDF]

The Astrophysical Journal Letters, 2020
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

After the Fall: The Dust and Gas in E+A Post-starburst Galaxies [PDF]

The Astrophysical Journal, 2018
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, J. D. T. Smith, D. A. Dale, K. D. French, K. V. Croxall, S. Zhukovska, A. Togi, E. F. Bell, A. F. Crocker, B. T. Draine, T. H. Jarrett, C. Tremonti, Yujin Yang, A. I. Zabludoff   +13 more
openaire   +4 more sources

AGN/Starburst Connection

Acta Polytechnica CTU Proceedings, 2014
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

Excess Of Post-Starburst Galaxies In Distant Galaxy Clusters

, 2017
I present a study on the impact of environment on galaxy evolution in distant galaxy clusters between redshifts 0.5 and 1.0. We find candidate galaxy clusters by applying a friends-of-friends algorithm to the deep photometric data of the UKIDSS Ultra-Deep Survey. Through studying the stellar mass functions, we reveal a strong excess of low-mass rapidly-
Socolovsky, Miguel, Almaini, Omar, Hatch, Nina   +2 more
openaire   +4 more sources

Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization

The Astrophysical Journal, 2023
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, Desika Narayanan, Qi Li, Romeel Davé   +3 more
doaj   +1 more source

Chemical Evolution of the Universe and its Consequences for Gravitational‐Wave Astrophysics

Annalen der Physik, Volume 536, Issue 2, February 2024.
Population properties of double compact object mergers (especially binary black holes) are sensitive to the metallicity dependent cosmic star formation history. The uncertainty of this quantity cannot be ignored and makes the interpretation of current gravitational wave observations difficult.
Martyna Chruślińska
wiley   +1 more source