HQ CAR IS A NEW W VIR TYPE STAR

Автор(и)

  • S. N. Udovichenko Astronomical Observatory, Odessa National University, Ukraine
  • V. V. Kovtyukh Astronomical Observatory, Odessa National University, Ukraine
  • I. A. Egorova European Southern Observatory, Chile
  • S. I. Belik Astronomical Observatory, Odessa National University,, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2013.26.82314

Ключові слова:

W Vir type Cepheids–stars, individual, HQCar

Анотація

HQ Car is listed as an  δ Cep star (DCEP) in the GCVS. High-resolution spectra of HQ Car showed the presence of the Balmer and HeI 5876  Å 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

Посилання

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Опубліковано

2013-11-07

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