The relation between RS CVn and Algol

Details The relation between RS CVn and Algol The relation between RS CVn and Algol

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ssrv...50..219h&link_type=abstract

(IAU, NSERC, Canadian Institute of Theoretical Astrophysics, et al., Colloquium on Algols, 107th, Sidney, Canada, Aug. 15-19, 19

Astronomy and Astrophysics

Astrophysics

111

Binary Stars, Late Stars, Starspots, Stellar Radiation, Stellar Rotation, X Rays, Companion Stars, Histograms, Infrared Radiation, Radio Emission, Stellar Orbits, Ultraviolet Radiation

Scientific paper

Rapidly rotating late-type secondaries in Algol binaries are examined with respect to the observed characteristics of CA stars. It is suggested that late-type secondaries in Algol binaries should be regarded as a separate class of CA stars. Ca II, H, and K emission cores are observed in the lobe-filling component of six semidetached binaries. It is shown that alternating period changes occur only in Algols that contain a late-type star.

Affiliated with

Also associated with

No associations

Rating

The relation between RS CVn and Algol does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The relation between RS CVn and Algol, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The relation between RS CVn and Algol will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1052463