1986
DOI: 10.1086/184659
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Spectroscopy of three Butcher-Oemler clusters of galaxies at a redshift of 0.2

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Cited by 57 publications
(62 citation statements)
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“…As such, they play an important part in understanding the evolutionary history of galaxy populations. Evidence for these (and related) galaxies have been found both locally (Caldwell et al 1993 ;Zabludo † et al 1996) and at moderate redshift (e.g., Sharples et al 1985 ;Lavery & Henry 1986 ;Couch & Sharples 1987 ;MacLaren, Ellis, & Couch 1988 ;Broadhurst et al 1988 ;Fabricant, McClintock, & Bautz 1991 ;Abraham et al 1996 ;Fisher et al 1998 ;Morris et al 1998 ;Dressler et al 1999), in both cluster and Ðeld environments. Many authors have interpreted the presence of these galaxies as evidence that a large percentage of cluster galaxies recently underwent strong starbursts (e.g., Dressler & Gunn 1983 ;Couch & Sharples 1987 ;Barger et al 1996 ;Poggianti & Barbaro 1996 ;Couch et al 1998 ;Poggianti et al 1999).…”
Section: Introductionmentioning
confidence: 95%
“…As such, they play an important part in understanding the evolutionary history of galaxy populations. Evidence for these (and related) galaxies have been found both locally (Caldwell et al 1993 ;Zabludo † et al 1996) and at moderate redshift (e.g., Sharples et al 1985 ;Lavery & Henry 1986 ;Couch & Sharples 1987 ;MacLaren, Ellis, & Couch 1988 ;Broadhurst et al 1988 ;Fabricant, McClintock, & Bautz 1991 ;Abraham et al 1996 ;Fisher et al 1998 ;Morris et al 1998 ;Dressler et al 1999), in both cluster and Ðeld environments. Many authors have interpreted the presence of these galaxies as evidence that a large percentage of cluster galaxies recently underwent strong starbursts (e.g., Dressler & Gunn 1983 ;Couch & Sharples 1987 ;Barger et al 1996 ;Poggianti & Barbaro 1996 ;Couch et al 1998 ;Poggianti et al 1999).…”
Section: Introductionmentioning
confidence: 95%
“…The second model is motivated by the interactions/mergers picture favoured by Lavery & Henry (1986) and Lacey & Silk (1991) in which encounters between close pairs of galaxies are responsible for the observed star formation in cluster galaxies at high redshift. We assume that a merger between galaxy-sized halos of roughly equal mass results in a burst of star formation.…”
Section: Models For Star Formation In Cluster Galaxiesmentioning
confidence: 99%
“…(Dressler & Gunn 1982, 1992Lavery & Henry 1986, 1988Fabricant et al 1991;Poggianti et al 1999Poggianti et al , 2006Ellingson et al 2001), has been extended to groups (Allington-Smith et al 1993;Wilman et al 2005a;Gerke et al 2007;Cucciati et al 2009b), and critically discussed in the context of selection biases (Andreon & Ettori 1999;Andreon et al 2004Andreon et al , 2006.…”
Section: Introductionmentioning
confidence: 99%