Further Remarks on the Cepheid RW Camelopardalis

Details Further Remarks on the Cepheid RW Camelopardalis Further Remarks on the Cepheid RW Camelopardalis

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aj....120..978f&link_type=abstract

The Astronomical Journal, Volume 120, Issue 2, pp. 978-978.

Astronomy and Astrophysics

Astronomy

1

Stars: Variables: Cepheids, Stars: Individual (Rw Camelopardalis), Stars: Population Ii

Scientific paper

A previous study of distinguishing between type I and type II Cepheids through the use of BV photometry found confusing results for RW Cam. This confusion is now found to be caused by RW Cam's having an unusually luminous binary companion, and the problem resolved. The criteria developed by Fernie & Ehlers are thus strengthened, and attention drawn to the role of companion stars in causing confusing results.

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