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Pulsation, Rotation and Mass Loss in Early-Type Stars
- Proceedings of the 162nd Symposium of the International Astronomical Union, Held in Antibes-Juan-Les-Pins, France, October 5-8, 1993
part of the International Astronomical Union Symposia series
- Binding:
- Paperback
- Pages:
- 550
- Published:
- August 30, 1994
- Edition:
- 11994
- Dimensions:
- 160x240x30 mm.
- Weight:
- 1031 g.
Delivery:
1-2 weeks
Expected delivery: December 12, 2024
Description of 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.
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