A stellar prominence in the white dwarf/red dwarf binary QS Vir: evidence for a detached system

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dc.contributor.authorParsons, S.
dc.contributor.authorTappert, Claus
dc.date.accessioned2016-05-10T18:14:47Z
dc.date.available2016-05-10T18:14:47Z
dc.date.issued2011
dc.identifier.doi10.1111/j.1365-2966.2010.18073.x
dc.identifier.issn0035-8711
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13431
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2010.18073.x
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society No. 4 (412), p. 2563-2570.
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas enanas blancases_ES
dc.subject.otherDiscos protoplanetarioses_ES
dc.subject.otherEstrellas binarias eclipsanteses_ES
dc.titleA stellar prominence in the white dwarf/red dwarf binary QS Vir: evidence for a detached systemes_ES
dc.typeartículo
sipa.codpersvinculados152942
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