Results 11 to 20 of about 30,724 (219)
Early-Type (E, S0) Galaxies in the Catalog of Isolated Galaxies (KIG) [PDF]
Astrophysical Bulletin, 2021 Accepted to Asrophysical Bulletin, 16 pages, 5 figures, 4 ...
Karachentseva, V. E. +2 more
openaire +2 more sources
Merger Signatures are Common, but not Universal, in Massive, Recently Quenched Galaxies at z ∼ 0.7
The Astrophysical Journal, 2023 We present visual classifications of merger-induced tidal disturbances in 143 M _* ∼ 10 ^11 M _⊙ post-starburst galaxies at z ∼ 0.7 identified in the $\mathrm{SQuIGG}\vec{L}{\rm{E}}$ Sample.
Margaret E. Verrico +11 more
doaj +1 more source
Formation and Evolution of E+A Galaxies in Dusty Starburst Galaxies
The Astrophysical Journal, 2001 The formation and evolution of the ``E+A'' (also named ``k+a'' and ``a+k'' types by Dressler et al. 1999) galaxies found in significant numbers in the cores of intermediate redshift clusters has been extensively discussed by many authors. In this paper, we model the spectral, dynamical and morphological evolution of a prime candidate for producing this
Bekki, Kenji +2 more
openaire +3 more sources
The Nature of E+A Galaxies in Intermediate‐Redshift Clusters [PDF]
The Astrophysical Journal, 2003 [Abridged] Combining HST/WFPC2 mosaics with extensive ground-based spectroscopy, we study the nature of E+A galaxies in three intermediate redshift clusters (z=0.33, 0.58, & 0.83). From a sample of ~500 confirmed cluster members, we isolate 46 E+A candidates to determine the E+A fraction and study their physical properties. We find E+A's comprise a
Tran, Kim-Vy +4 more
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“E+A” Galaxies: Environment and Evolution [PDF]
Symposium - International Astronomical Union, 1999 One important approach to the study of galaxy evolution is to identify those galaxies whose spectral and/or morphological characteristics suggest that they are in transition. For example, “E+A” galaxies, which have strong Balmer absorption lines and no significant [OII] emission, are generally interpreted as post-starburst galaxies in which the star ...
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The H
The Astrophysical Journal, 2006 We present deep single-dish HI observations of a sample of six nearby E+A galaxies (0 ...
Buyle, Pieter +5 more
openaire +4 more sources
The Environment of ``E+A'' Galaxies
The Astrophysical Journal, 1996 39 uuencoded, compressed pages (except Fig 1), complete preprint at ftp://ociw.edu/pub/aiz/eplusa.ps, ApJ ...
Zabludoff, A. I. +7 more
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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 +3 more
openaire +1 more source
Early assembly of the most massive galaxies [PDF]
, 2009 The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging(1).
Chris A. Collins +53 more
core +1 more source
E+A Galaxies: Did They Lose The A to Become E? [PDF]
Proceedings of the International Astronomical Union, 2006 AbstractWe present deep HI observations of a sample of 9 nearby E+A galaxies (0.05 < z < 0.1). In 7 of them, we detected up to a few times 109 M⊙ of neutral gas, making the link between E+As and early-types less direct than previously thought.
Sven De Rijcke +5 more
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