Heavily obscured quasar host galaxies at z ∼ 2 are discs, not major mergers.

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dc.contributor.authorSchawinski, Kevin
dc.contributor.authorTreister, Ezequiel
dc.contributor.authorSimmons, Brooke D.
dc.contributor.authorUrry, C. Meg
dc.contributor.authorGlikman, Eilat
dc.date.accessioned2019-05-24T15:08:18Z
dc.date.available2019-05-24T15:08:18Z
dc.date.issued2012
dc.date.updated2019-05-24T15:07:07Z
dc.fuente.origenORCID
dc.identifier.doi10.1111/j.1745-3933.2012.01302.x
dc.identifier.issn1745-3933
dc.identifier.urihttps://ui.adsabs.harvard.edu/#abs/2012MNRAS.425L..61S
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/22868
dc.issue.numeroNo. 1
dc.language.isoen
dc.pagina.finalL65
dc.pagina.inicioL61
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society, Letters, vol. 425, no. 1 (sep. 2012), pp. L61-L65.
dc.revistaMonthly Notices of the Royal Astronomical Society: Letterses_ES
dc.subjectGalaxies: activees_ES
dc.subjectGalaxies: high-redshiftes_ES
dc.subjectGalaxies: Seyfertes_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleHeavily obscured quasar host galaxies at z ∼ 2 are discs, not major mergers.es_ES
dc.typeartículo
dc.volumenVol. 425
sipa.codpersvinculados1031846
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