[PDF] Top 20 The evolution of post starburst galaxies from z=2 to 0 5
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The evolution of post starburst galaxies from z=2 to 0 5
... the evolution of the populations can be ob- tained from the galaxy stellar mass ...apart from the lowest red- shift PSB bin, for which the upturn at lower stellar masses required a double Schechter ... See full document
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The evolution of post starburst galaxies from z=2 to 0 5
... quiescent galaxies out to redshifts of z ∼ 4 or more ...quiescent galaxies are found to be elliptical and highly compact ...the galaxies (Hopkins et ...gas from the system ... See full document
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The structure of post starburst galaxies at 0 5 < z < 2: evidence for two distinct quenching routes at different epochs
... ( z < ...at z > 1, several studies have reported centrally-concentrated young stellar populations in these galaxies ...high- z PSBs does not necessarily rule out a gas-rich merger ... See full document
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The structure of post starburst galaxies at 0 5 < z < 2 : evidence for two distinct quenching routes at different epochs
... < z < 1) have not experienced a major disruption to their stellar distribution ...these galaxies have experienced a violent ‘compaction’ ...these galaxies are simply quietly transitioning into ... See full document
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Evolution of the cold gas properties of simulated post starburst galaxies
... field galaxies and are thought to play a role in triggering the starbursts that initiate the formation of PSBs ...were 2:1 mergers or ...extreme starburst, but also by the loss of gas in other ways, ... See full document
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The origin and fate of post starburst galaxies : morphological and structural image analysis of local galaxies with recent episodes of enhanced star formation
... of post-starburst galaxies representing a link between the star-forming and passive phases of galaxy evolution is supported by results of many studies, which found that the mor- phological and ... See full document
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The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... sive galaxies predominantly inhabit denser environments and galaxy clusters, whereas star-forming systems are mostly found in the ...star-forming galaxies is higher in more distant clusters than those in ... See full document
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The enhancement of rapidly quenched galaxies in distant clusters at 0 5 < z < 1 0
... galaxy evolution in the red- shift range 0.5 < z < ...quenched galaxies in cluster environments compared to the ...star-forming galaxies, which show a sharp radial decline towards ... See full document
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The origins of post starburst galaxies at z < 0 05
... ‘K+A’ galaxies, many studies agree that they are likely transitioning between the blue cloud and the red sequence, both in clusters and in the ...passive galaxies in the local field underwent a ‘K+A’ phase ... See full document
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Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z <0 5
... of galaxies at high ...of galaxies as: chains, doubles, tadpoles, clump-clusters, spirals, and ...chain galaxies with those of clump-cluster ...of galaxies but seen from di ff erent ... See full document
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The evolution of the cold interstellar medium in galaxies following a starburst
... the galaxies, ...galaxy evolution (Yan et ...(i.e. starburst age and burst strength), we can select a complete sample of objects in a physically meaningful ...Section 2, we describe the method ... See full document
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Evolution of starburst galaxies in the Illustris simulation
... that starburst galaxies are triggered by inter- action ...of starburst galaxies to determine if this could be why we witness a bimodality in post-starburst populations within ... See full document
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The Evolutionary Sequence of Post Starburst Galaxies
... < z < 0.8) E+A galaxies are predominantly in clus- ters where the star-formation has been quenched on a short time scale of 1 ...E+A galaxies are located in other environments such as the field ... See full document
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The diverse evolutionary pathways of post starburst galaxies
... Simulated galaxies in the z = ...the post-starburst phase closely resembling those conjectured from observational ...two galaxies can cause a powerful starburst and ... See full document
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Post starburst galaxies in SDSS IV MaNGA
... PSB galaxies (Section ...of z > ...a starburst or the strong Balmer absorption lines seen in post- starburst galaxies, or whether an AGN is necessary or able to halt the ... See full document
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Disc colours in field and cluster spiral galaxies at 0 5 ≲z≲ 0 8
... . z . 0.8. Our cluster sample contains 172 spiral galaxies, and our control sample is composed of 96 field disc ...spiral galaxies have disc V − I colours redder by more than 1σ of the mean colours ... See full document
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The properties of post starburst galaxies from spectral fitting
... with galaxies spectra, one should always account for the effect of dust in the interstellar media (ISM) and the dust that surrounds newborn ...emission from young stars with temperatures > 10000 K, O and ... See full document
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The LOFAR window on star forming galaxies and AGNs – curved radio SEDs and IR–radio correlation at 0<z<2 5
... (SF) galaxies and active galactic nuclei (AGNs) up to redshift z = ...emission from 150 MHz to ...1542 galaxies in ∼7 deg 2 of the LOFAR Bo¨otes ...their evolution across cosmic ... See full document
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The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... individual galaxies leaking LyC photons by matching our Clean galaxy sample with the public GALEX EM cleaned catalogue ...and 2/5 LAEs as reliable candidate LyC ...HAEs, 2 LAEs) the N U V ... See full document
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Clumpy galaxies in CANDELS II Physical properties of UV bright clumps at 0 5 ≤ z < 3
... An important test of different clump evolution models is the age gradient. The inward migration scenario ( e.g., Bournaud et al. 2007; Elmegreen et al. 2008; Ceverino et al. 2010; Bournaud et al. 2014; Mandelker ... See full document
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