Results 11 to 20 of about 181 (148)
Stars, Gas, and Star Formation of Distant Post-starburst Galaxies
The Astrophysical Journal, 2023 We present a comprehensive multiwavelength study of five post-starburst galaxies with M _* > 10 ^11 M _⊙ at z ∼ 0.7, examining their stars, gas, and current and past star formation activities.
Po-Feng Wu +7 more
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Spatially Resolved Kinematics of Post-starburst Galaxies
The Astrophysical JournalStar-forming galaxies can reach quiescence via rapid transition through merger-triggered starbursts that consequently affect both their kinematics and star formation rates.
Bhavya Pardasani, K. Decker French
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The Evolution of the Interstellar Medium in Post-starburst Galaxies [PDF]
The Astrophysical Journal, 2019 Abstract We derive dust masses (M dust) from the spectral energy distributions of 58 post-starburst galaxies (PSBs). There is an anticorrelation between specific dust mass (M dust/M ⋆) and the time elapsed since the starburst ended, indicating that dust was either destroyed, expelled,
Zhihui Li +3 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 and the transformation of blue into red galaxies [PDF]
Astronomische Nachrichten, 2009 AbstractWe present deep single‐dish radio observations of a sample of nearby post‐starburst galaxies (0.05 < z < 0.1). About 50% of these post‐starburst galaxies are detected at 21 cm, with HI masses of ∼109 M⊙, up to ∼1010 M⊙. These post‐starburst galaxies are as gas‐rich as spiral galaxies with comparable luminosities. There appears to exist no
De Rijcke, Sven +4 more
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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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