Relativistic mergers of black hole binaries have large, similar masses, low spins and are circular

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dc.contributor.authorAmaro Seoane, Pau
dc.contributor.authorChen, Xian
dc.date.accessioned2021-05-13T17:51:30Z
dc.date.available2021-05-13T17:51:30Z
dc.date.issued2016
dc.format.extent8 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stw503
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stw503
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/58356
dc.issue.numeroNo. 3
dc.language.isoen
dc.nota.accesoContenido parcial
dc.pagina.final3082
dc.pagina.inicio3075
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso restringido
dc.titleRelativistic mergers of black hole binaries have large, similar masses, low spins and are circulares_ES
dc.typeartículo
dc.volumenVol. 458
sipa.codpersvinculados1015435
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