Results 121 to 130 of about 10,366 (216)
Environmental variation of the low-mass IMF. [PDF]
Tanvir TS, Krumholz MR, Federrath C.
europepmc +1 more source
Optical and near infrared photometry of Butcher-Oemler clusters [PDF]
Rich clusters of galaxies at moderate redshifts (z approx. .3) have a larger proportion of optically blue galaxies than their low redshift counterparts.
Rieke, Marcia J., Shier, Lisa M.
core +1 more source
Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to a decrease of cold gas. In the first paper we showed that the dust removal timescale in early-type galaxies (ETGs) is about 2.5 Gyr.
Michał J. Michałowski +17 more
doaj +1 more source
Some Die Filthy Rich: The Diverse Molecular Gas Contents of Post-starburst Galaxies Probed by Dust Absorption [PDF]
Hassen M. Yesuf, Luis C. Ho
openalex +1 more source
Gas excitation of post-starburst galaxies at 0.6 < z < 1.3 [PDF]
A. Zanella +3 more
openalex +1 more source
The confirmation of massive quiescent galaxies emerging within the first billion years of the Universe poses intriguing questions about the mechanisms of galaxy formation.
Po-Feng Wu
doaj +1 more source
Evidence of ongoing AGN-driven feedback in a quiescent post-starburst E+A galaxy [PDF]
Dalya Baron +4 more
openalex +1 more source
Shocked POstarburst Galaxies (SPOGs) exhibit both emission lines suggestive of shock-heated gas and poststarburst-like stellar absorption, resulting in a unique subset for galaxy evolution studies.
Antoniu Fodor +15 more
doaj +1 more source
We report the spectroscopic detection of neutral gas inflow into a massive ( M _* ≃ 4 × 10 ^10 M _⊙ ) quiescent galaxy observed at z _spec = 2.6576 with the James Webb Space Telescope (JWST).
Davide Bevacqua +18 more
doaj +1 more source
A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6 [PDF]
Masafusa Onoue +47 more
openalex +1 more source

