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Pulsation, Rotation and Mass Loss in Early-Type Stars
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Pulsation, Rotation and Mass Loss in Early-Type Stars

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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