A z=0.9 supercluster of X-ray luminous, optically selected, massive galaxy clusters
dc.contributor.author | Gilbank, D. | |
dc.contributor.author | Barrientos, Luis Felipe | |
dc.date.accessioned | 2017-04-11T20:50:46Z | |
dc.date.available | 2017-04-11T20:50:46Z | |
dc.date.issued | 2008 | |
dc.identifier.doi | 10.1086/588138 | |
dc.identifier.issn | 2041-8205 | |
dc.identifier.uri | https://doi.org/10.1086/588138 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/18693 | |
dc.language.iso | en | |
dc.nota.acceso | contenido completo | |
dc.relation.isformatof | The Astrophysical Journal Letters. Vol. 677, no. 2 (2008), p. [L89]-L92 | |
dc.revista | The Astrophysical Journal Letters | es_ES |
dc.rights | acceso abierto | |
dc.subject.ddc | 520 | |
dc.subject.dewey | Astronomía | es_ES |
dc.subject.other | Cúmulos de galaxias | es_ES |
dc.subject.other | Astronomía de rayos X | es_ES |
dc.subject.other | Espectroscopía astronómica | es_ES |
dc.title | A z=0.9 supercluster of X-ray luminous, optically selected, massive galaxy clusters | es_ES |
dc.type | artículo | |
dc.volumen | Vol. 677 | |
sipa.codpersvinculados | 102167 |
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