HQ Car is a new W Vir type star

dc.contributor.authorUdovichenko, Serhii M.en
dc.contributor.authorKovtyukh, ValeryV.en
dc.contributor.authorEgorova, I. A.en
dc.contributor.authorBelik, S. I.en
dc.contributor.authorУдовіченко, Сергій Миколайовичuk
dc.contributor.authorКовтюх, Валерій Володимировичuk
dc.date.accessioned2014-03-28T08:07:54Z
dc.date.available2014-03-28T08:07:54Z
dc.date.issued2013
dc.description.abstractHQ Car is listed as an Cep star (DCEP) in the GCVS. High-resolution spectra of HQ Car showed the presence of the Balmer and He I 5876˚A emissions. The light curve shows steeper rise than decline, and there is evidence for the presence of a bump in the descending branch around the phase of 0.4. From considerations of the period, spectral type, presence of the bump, Helium and Balmer emissions we conclude that HQ Car belongs to the W Vir class of Type II Cepheids.en
dc.identifier.citationOdessa Astronomical Publicationsen
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4783
dc.language.isoen
dc.publisherAstroprinten
dc.relation.ispartofseries;vol. 26, issue 1, p. 120-122
dc.subjectW Vir type Cepheidsen
dc.subjectstars: individual: HQ Caren
dc.titleHQ Car is a new W Vir type staren
dc.typeArticleen
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