A z=0.9 supercluster of X-ray luminous, optically selected, massive galaxy clusters

dc.contributor.authorGilbank, D.
dc.contributor.authorBarrientos, Luis Felipe
dc.date.accessioned2017-04-11T20:50:46Z
dc.date.available2017-04-11T20:50:46Z
dc.date.issued2008
dc.identifier.doi10.1086/588138
dc.identifier.issn2041-8205
dc.identifier.urihttps://doi.org/10.1086/588138
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/18693
dc.language.isoen
dc.nota.accesocontenido completo
dc.relation.isformatofThe Astrophysical Journal Letters. Vol. 677, no. 2 (2008), p. [L89]-L92
dc.revistaThe Astrophysical Journal Letterses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherCúmulos de galaxiases_ES
dc.subject.otherAstronomía de rayos Xes_ES
dc.subject.otherEspectroscopía astronómicaes_ES
dc.titleA z=0.9 supercluster of X-ray luminous, optically selected, massive galaxy clusterses_ES
dc.typeartículo
dc.volumenVol. 677
sipa.codpersvinculados102167
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