A transient sub-eddington black hole x-ray binary candidate in the dust lanes of centaurus a

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dc.contributor.authorBurke, M.
dc.contributor.authorJordán Colzani, Andrés Cristóbal
dc.date.accessioned2016-05-10T18:02:12Z
dc.date.available2016-05-10T18:02:12Z
dc.date.issued2012
dc.identifier.doi10.1088/0004-637X/749/2/112
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12136
dc.identifier.urihttps://doi.org/10.1088/0004-637X/749/2/112
dc.language.isoen
dc.relation.isformatofAstrophysical Journal No. 2 (749), Art. 112.
dc.revistaAstrophysical Journales_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherAgujeros negroses_ES
dc.subject.otherEstrellas de neutroneses_ES
dc.subject.otherEstrellas - Masases_ES
dc.subject.otherAstronomía de rayos Xes_ES
dc.titleA transient sub-eddington black hole x-ray binary candidate in the dust lanes of centaurus aes_ES
dc.typeartículo
sipa.codpersvinculados176960
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