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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-Jua

Pulsation, Rotation and Mass Loss in Early-Type Stars: Proceedings of the 162nd Symposium of the International Astronomical Union, Held in Antibes-Jua

Paperback

Series: International Astronomical Union Symposia, Book 162

Astronomy & SpacePhysics

ISBN10: 0792330455
ISBN13: 9780792330455
Publisher: Springer Nature
Published: Aug 31 1994
Pages: 550
Weight: 1.75
Height: 1.17 Width: 6.14 Depth: 9.21
Language: English
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. Thanks to advances in digital spectroscopy, new types of pulsating B stars have been discovered. The pulsations can be understood in terms of the recent revision of metal opacities, but the effects of rapid rotation and magnetic fields need further study. Observations in the UV and X-ray regions demonstrate that many B and Be stars show other activity, besides pulsation which is not yet understood. The reason for the enhanced mass loss in Be stars is a question which dominates the Symposium and which remains unanswered, although it is surely to be found in activity at or near the photosphere coupled with rotation. It is shown that the geometry of the circumstellar envelopes around Be stars is indeed a flattened disk as they can now be optically resolved. The variability of radiatively-driven winds from O and B stars are likely related to the rotation of the star. This underlines the central theme of the book: that the various phenomena seen in these stars cannot be studied in isolation.

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