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Pulsation, Rotation and Mass Loss in Early-Type Stars
In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together for the first time in order to broaden our understanding of O and B stars. The variability of radiatively-driven winds from O and B stars are likely related to the rotation of the star.
- Undertitel
- Proceedings of the 162nd Symposium of the International Astronomical Union, Held in Antibes-Juan-Les-Pins, France, October 5–8, 1993
- Upplaga
- Softcover reprint of the original 1st ed. 1994
- ISBN
- 9780792330455
- Språk
- Engelska
- Vikt
- 310 gram
- Utgivningsdatum
- 1994-08-31
- Förlag
- Springer
- Sidor
- 550
