HQ CAR IS A NEW W VIR TYPE STAR

dc.contributor.authorUdovichenko, S. N.
dc.contributor.authorKovtyukh, Valery V.
dc.contributor.authorEgorova, I. A.
dc.contributor.authorBelik, S. I.
dc.date.accessioned2014-03-28T08:07:54Z
dc.date.available2014-03-28T08:07:54Z
dc.date.issued2013
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/1.uk
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.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4783
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 26, issue 1, p. 120-122
dc.subjectW Vir type Cepheids – starsuk
dc.subjectindividualuk
dc.subjectHQ Caruk
dc.titleHQ CAR IS A NEW W VIR TYPE STARuk
dc.typeArticleuk
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