This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

THE MAGNETIC, SPECTRUM, AND PHOTOMETRIC VARIATIONS OF THE AP STAR 52 HERCULIS.

and

© 1978. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
, , Citation S. C. Wolff and G. W. Preston 1978 PASP 90 406 DOI 10.1086/130348

Download Article PDF

Article metrics

57 Total downloads

Share this article

Author affiliations

1 Hawaii, University, Honolulu, Hawaii

2 Hale Observatoires, Pasadena, Calif.

Buy this article in print

Journal RSS
Sign up for new issue notifications
1538-3873/90/536/406

ABSTRACT

The strength of Ca ii N3933, the magnetic field intensity, and the brightness of 52 Her all vary periodically in a period of 3.8575 days. Narrow-band ( 10 A) photometry of the K line appears to be a very effective way to determine periods for cool Ap stars with broad lines. Key words: magnetic star-variable star-absorption-line variations

Export citation and abstract BibTeX RIS

Previous article in issue
Next article in issue
10.1086/130348