A Group of Red, Ly-alpha Emitting, High Redshift Galaxies

dc.contributor.authorFrancis, Paul
dc.contributor.authorWoodgate, Bruce E.
dc.contributor.authorDanks, Anthony C.
dc.date.accessioned2018-09-07T06:28:51Z
dc.date.available2018-09-07T06:28:51Z
dc.date.issued1997-03-27
dc.description.abstractWe have discovered two new high redshift (z=2.38) galaxies, near the previously known z=2.38 galaxy 2139-4434 B1 (Francis et al. 1996). All three galaxies are strong Ly-alpha emitters, and have much redder continuum colors (I-K about 5) than other optically-selected high redshift galaxies. We hypothesize that these three galaxies are QSO IIs; radio-quiet counterparts of high redshift radio galaxies, containing concealed QSO nuclei. The red colors are most easily modelled by an old (> 0.5 Gyr), massive (> 10E11 solar masses) stellar population. If true, this implies that at least one galaxy cluster of mass much greater than 3E11 solar masses had collapsed before redshift five.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/147238
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0004-637X/..."author can archive publisher's version/PDF" from SHERPA/RoMEO site (as at 7/09/18)en_AU
dc.sourceThe Astrophysical Journalen_AU
dc.titleA Group of Red, Ly-alpha Emitting, High Redshift Galaxiesen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1en_AU
local.bibliographicCitation.lastpageL28en_AU
local.bibliographicCitation.startpageL25en_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoremailPaul.Francis@anu.edu.auen_AU
local.contributor.authoruidu9710753en_AU
local.identifier.citationvolume482en_AU
local.identifier.doi10.1086/310667en_AU
local.identifier.uidSubmittedByu1005913en_AU
local.publisher.urlhttps://aas.org/en_AU
local.type.statusPublished Versionen_AU

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