Results 21 to 30 of about 6,393 (178)
The star formation histories of z ∼ 1 post-starburst galaxies [PDF]
, 2022 Funding: LTA acknowledges support from the Ministry of Higher Education and Scientific Research (MOHESR), Iraq. AW acknowledges financial support from the Royal Society Newton Fund (grant NAF/R1/180403, PI Natalia Vale Asari) and Fundação de à Amparo ...
Wilkinson, Aaron +13 more
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The Ages of Starbursts in Post-Starburst Galaxies [PDF]
The Astronomical Journal, 1996 14 pages + 7 figures, uuencoded gzipped postscript.
Leonardi, Andrew J., Rose, James A.
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LOFAR Detection of Post-starburst Galaxies
Research Notes of the AAS, 2023 Abstract We report detection of 104 radio counterparts in a sample of 1204 Sloan Digital Sky Survey-detected post-starburst (PSB) galaxies using the 144 MHz LOw-Frequency ARray (LOFAR) Two-meter Sky Survey Data Release 2 (LoTSS2). The detection rate of optically selected PSB galaxies in the 144 MHz images is ∼8.6% while that in the 1.4 ...
Riya Mullick, Amitesh Omar
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CO-Observations of Post-Starburst Galaxies
Astrophysics and Space Science, 2001 The so-called starburst phenomenon is an issue of great importance for the evolution of galaxies. Although a lot of progress has been made in this field, it is still unknown how they evolve.
Barden, M +3 more
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AGB populations in post-starburst galaxies [PDF]
Astronomy & Astrophysics, 2014 In a previous paper we compared the SEDs of a sample of 808 K+A galaxies from the FUV to the MIR to the predictions of the spectrum synthesis models explicitly using AGB components. Here we use the new AGB-light models from C. Maraston (including less fuel for the later stages of stellar evolution and improved calibrations) to address the discrepancies
Melnick, J., De Propris, R.
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The Typical Massive Quiescent Galaxy at z ∼ 3 is a Post-starburst [PDF]
The Astrophysical Journal Letters, 2020 Abstract We have obtained spectroscopic confirmation with Hubble Space Telescope WFC3/G141 of a first sizeable sample of nine quiescent galaxies at 2.4 < z < 3.3. Their average near-UV/optical rest-frame spectrum is characterized by low attenuation (AV ∼ 0.6 mag) and a strong Balmer break, larger than the 4000 Å ...
C. D’Eugenio +12 more
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Post-Starburst Galaxies in Clusters from the GASP Survey. [PDF]
, 2022 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
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Evolution Through the Post-starburst Phase: Using Post-starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution [PDF]
Publications of the Astronomical Society of the Pacific, 2021 Post-starburst (or "E+A") galaxies trace the fastest and most dramatic processes in galaxy evolution. Recent work studying the evolution of galaxies through this phase have revealed insights on how galaxies undergo structural and stellar population changes as well as the role of various feedback mechanisms.
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Post-starburst Galaxies in the Centers of Intermediate-redshift Clusters
The Astrophysical Journal, 2022 Abstract We present results from MUSE spatially resolved spectroscopy of 21 post-starburst galaxies in the centers of eight clusters from z ∼ 0.3 to z ∼ 0.4. We measure spatially resolved star formation histories (SFHs), the time since quenching (t Q ), and the fraction of stellar
Ariel Werle +19 more
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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/ +11 more
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