X-Ray Astronomy in the Exosat Era Proceedings of the XVIII ESLAB Sysmposium, held in The Hague, The Netherlands, 5–9 November 1984
Algol is a triple system containing a 70 hr eclipsing binary (K IV and B8 V) in a 694 day orbit with an A V star. The X-ray emission from this system (Schnopper et al 1976) is thought to be associated with a corona surrounding the lobe filling and synchron ously rotating K IV star. This is based on...
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| Format: | eBook |
| Language: | English |
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Dordrecht
Springer Netherlands
1985, 1985
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| Edition: | 1st ed. 1985 |
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| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- I / Galactic X-Ray Astronomy
- Section I: Stellar Coronae and Isolated White Dwarfs
- Section II: Cataclysmic Variables
- Section III: X-Ray Binary Sources — Low Mass/High Mass Systems
- Section IV: Supernova Remnants and the Interstellar Medium
- II / Extragalactic X-Ray Astronomy
- Section V: Active Galactic Nuclei
- Section VI: Clusters of Galaxies
- Section VII: Other Extragalactic Topics
- III
- Section VIII: Instrumentation/General Interest
- Index of Names
- Index of Subjects