Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/4783
Title: HQ CAR IS A NEW W VIR TYPE STAR
Authors: Udovichenko, S. N.
Kovtyukh, Valery V.
Egorova, I. A.
Belik, S. I.
Citation: Odessa Astronomical Publications
Issue Date: 2013
Publisher: Astroprint
Keywords: W Vir type Cepheids – stars
individual
HQ Car
Series/Report no.: ;vol. 26, issue 1, p. 120-122
Abstract: HQ 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.
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/1.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/4783
Appears in Collections:Odessa Astronomical Publications

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