Results 101 to 110 of about 5,089,625 (177)
Context. Galaxies may suffer some starburst and quenched periods in their history due to galaxy mergers and feedback. However, semi-numerical simulations of the Epoch of Reionization (EoR) do not accurately model the effects of the star formation history
Ma Qing-Bo +8 more
doaj +1 more source
Post-starburst galaxies in the COSMOS field at z < 0.45
Post-starburst galaxies (PSBs) are key to understanding how galaxies transition from active star formation to quiescence. We identify 36 PSBs by spectroscopic selection in the COSMOS field at z < 0.45.
D.J. Pisano, Martin Shanobe
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Post-starburst (PSB) galaxies, having recently experienced a starburst followed by rapid quenching, are excellent laboratories to probe physical mechanisms that drive starbursts and shutting down of star formation. Integral-field spectroscopy reveals the
Yirui Zheng +17 more
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James Webb Space Telescope (JWST) has revealed temporarily quenched and ultraviolet-luminous galaxies in the early Universe, suggesting enhanced star formation stochasticity. Verifying this hypothesis is critical yet challenging.
Bingjie Wang +15 more
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We investigate the effects of ram-pressure stripping on four galaxies within the massive, strong-lensing cluster MACS-J0138.0-2155 ($z=0.336$). Of these, three are classified as jellyfish galaxies, with significant elongated tails. Two of these jellyfish
Catherine C. Gibson +2 more
doaj +1 more source
The mystery of unidentified infrared emission bands. [PDF]
Kwok S.
europepmc +1 more source
Quiescent Host Galaxies of Extended Quasars Revealed by Spectrophotometric Decomposition
Previous works of low-redshift quasar host galaxies have focused on compact quasars and found that their host galaxies are mainly star-forming galaxies.
Shengxiu Sun +29 more
doaj +1 more source
Post-Starburst Galaxies in Clusters from the GASP Survey.
Post-starburst galaxies, also known as k+a galaxies, show no sign of emission lines and prominent Balmer absorption lines in their spectra. They are in a transitional phase between the star forming and the passive galaxies. I present here the study of a
Santorelli, Maria
core
Environmental variation of the low-mass IMF. [PDF]
Tanvir TS, Krumholz MR, Federrath C.
europepmc +1 more source
New Methods for Tracking Galaxy and Black Hole Evolution Using Post-Starburst Galaxies
Galaxies in transition from star-forming to quiescence are a natural laboratory for exploring the processes responsible for this evolution. Using a sample of post-starburst galaxies identified to have recently experienced a recent burst of star formation
French, Katheryn Decker
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