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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2743
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.date.accessioned2008-07-18T05:53:36Z-
dc.date.available2008-07-18T05:53:36Z-
dc.date.issued1993-06-
dc.identifier.citationPublications of the Astronomical Society of the Pacific, Vol. 105, No. 688, pp. 574 - 577en
dc.identifier.issn0004-6280-
dc.identifier.urihttp://hdl.handle.net/2248/2743-
dc.description.abstractAn identification of V482 Cygni, a R Coronae Borealis star, with a quadruple system containing a K5 III star is rejected. High-resolution spectra show that the radial velocity of V482 Cyg and the K5 III star differ by 35 km/s, and the interstellar NaD lines are much stronger in the spectrum of V482 Cyg. These observations suggest that V482 Cyg is much more distant than the K5 III star and has an absolute magnitude of M(V) about -5, similar to that of R Coronae Borealis stars in the LMC.en
dc.format.extent515804 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993PASP..105..574Ren
dc.subjectMagellanic cloudsen
dc.subjectRadial velocityen
dc.subjectStellar magnitudeen
dc.subjectStellar spectraen
dc.subjectVariable starsen
dc.subjectH alpha lineen
dc.subjectPixelsen
dc.subjectSpectral resolutionen
dc.titleOn the absolute magnitude of V482 Cygni, an R Coronae Borealis staren
dc.typeArticleen
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