Hostname: page-component-f554764f5-8cg97 Total loading time: 0 Render date: 2025-04-22T00:44:14.677Z Has data issue: false hasContentIssue false
  • English
  • Français

Variability Studies and Asteroseismology with the XMM Optical Monitor

Published online by Cambridge University Press:  12 April 2016

S. Horner  and
E. Antonello
S. Horner
Affiliation:
Department of Astronomy and Astrophysics, Penn State University, University Park, PA 16802, USA
E. Antonello
Affiliation:
Osservatorio Astronomico di Brera, Milano-Merate, Italy

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.

It will be possible to make photometric variability studies from space of stars serendipitously falling in the field of view of the Optical Monitor, and to search for asteroseismological phenomena in bright target stars.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 457 - 458
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Antonello, E., & Cropper, M.S. 1992, in Stellar Photometry - Current Techniques and Future Developments, Butler, C.J., Elliott, I., Cambridge Univ. Press, 358 Google Scholar
Homer, S.D., et al. 1994, in Instrumentation in Astronomy VIII, Crawford, D.L., Craine, E.R., SPIE, 2198, 1238 Google Scholar
Jenkner, H., et al. 1990, ApJ, 99, 2081 Google Scholar
Lasker, B.M., et al. 1988, ApJS, 68, 1 Google Scholar
Mason, K.O., et al. 1995, Adv. Space Res., 16, 41 CrossRefGoogle Scholar