Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-19T07:21:00.376Z Has data issue: false hasContentIssue false
  • English
  • Français

Short-term Photometric Variability in Be Stars in the Far-Ultraviolet - A Preliminary Report

Published online by Cambridge University Press:  23 September 2016

R. S. Polidan  and
G. J. Peters
R. S. Polidan
Affiliation:
Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 8S721, USA
G. J. Peters
Affiliation:
Space Sciences Center University of Southern California Los Angeles, CA 90089, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this paper we report preliminary results on the first search for short term photometric variations in the far-UV in Be stars. Results for mu Cen and 28 Cyg indicate no significant variations.

Type
III. The Circumstellar Gas
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 282 - 285
Copyright
Copyright © Cambridge University Press 1987

References

Broadfoot, A. L. (1977). Space Sci. Rev., 21, 183.Google Scholar
Broadfoot, A. L. (1981). J. Geophys. Res., 86, 8259.Google Scholar
Drilling, J. S., Holberg, J. B., and Schoenberner, D. (1984). Astrophys. J., 283, L67.Google Scholar
Holberg, J. B., Forrester, W. T., Shemansky, D. E., and Barry, D. C. (1982). Astrophys. J., 257, 650.Google Scholar
Percy, J. B. (1986). Highlights of Astronomy, in press.Google Scholar
Polidan, R. S., Stalio, R. and Peters, G. J. (1987). Astrophys. J in press.Google Scholar