The evolutionary status of V627 CAS

Details The evolutionary status of V627 CAS The evolutionary status of V627 CAS

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..616b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, July 1988, p. 616-622. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Binary Stars, Cool Stars, Dwarf Stars, Hot Stars, Red Giant Stars, Stellar Evolution, Ubv Spectra, Ultraviolet Radiation

Scientific paper

Results of photometric (UBVRIJHK) and polarimetric (RI) observations of V627 Cas which were performed during 1985-1988 are presented. The data suggest that V627 Cas is a binary star consisting of a cold red giant and a hot dwarf. It is expected that the object emits more UV radiation at wavelengths less than 3000 A. It is believed that V627 is at a late evolutionary stage.

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