Spectroscopic classification of cataclysmic variable candidates

Simple item page
dc.contributor.authorSchmidtobreick, L
dc.contributor.authorGalli, L
dc.contributor.authorWhiting, A
dc.contributor.authorTappert, C
dc.contributor.authorCarver, AJ
dc.date.accessioned2025-01-21T01:06:47Z
dc.date.available2025-01-21T01:06:47Z
dc.date.issued2005
dc.description.abstractWe present low-resolution optical spectroscopy for six cataclysmic variable candidates and the old nova V888 Cen. We confirm the classification as cataclysmic variable for LB 9963 and FQ Mon, while the other four candidates turn out to be different types of stars. We discuss the individual spectra and pay special attention to the mass transfer rate and disk temperature and density of the three cataclysmic variables.
dc.fuente.origenWOS
dc.identifier.eissn1538-3873
dc.identifier.issn0004-6280
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/96223
dc.identifier.wosidWOS:000231451100007
dc.issue.numero835
dc.language.isoen
dc.pagina.final949
dc.pagina.inicio944
dc.revistaPublications of the astronomical society of the pacific
dc.rightsacceso restringido
dc.titleSpectroscopic classification of cataclysmic variable candidates
dc.typeartículo
dc.volumen117
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
Files
Collections
Artículos de revistas