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Springer, 1994-08-31. Paperback. New. 1.3000 in x 9.4500 in x 6.3000 in.
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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 Paperback - 1994 - 1st Edition
by Luis A. Balona (Editor); Huib F. Henrichs (Editor); Jean Michel Le Contel (Editor)
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- Title Pulsation, Rotation and Mass Loss in Early-Type Stars: Proceedings of the 162nd Symposium of the International Astronomical Union, Held in Antibes-Jua
- Author Luis A. Balona (Editor); Huib F. Henrichs (Editor); Jean Michel Le Contel (Editor)
- Binding Paperback
- Edition number 1st
- Edition 1
- Pages 550
- Volumes 1
- Language ENG
- Publisher Springer
- Date 1994-08-31
- ISBN 9780792330455 / 0792330455
- Weight 1.75 lbs (0.79 kg)
- Dimensions 9.21 x 6.14 x 1.17 in (23.39 x 15.60 x 2.97 cm)
- Dewey Decimal Code 523.88
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Pulsation, Rotation and Mass (International Astronomical Union Symposia)
by L.A. Balona , H.F. Henrichs
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Kluwer Academic Publishers, 1994. Paperback. New. Usually Dispatched within 1-2 Business Days , Buy with confidence , excellent customer service
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Pulsation, Rotation and Mass Loss in Early-Type Stars
by Luis A. Balona
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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
by Luis A. Balona
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Paperback / softback. New. 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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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
by Luis A. Balona
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Paperback / softback. New. 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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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
by Balona, Luis A. (Editor) / Henrichs, Huib F. (Editor) / Le Contel, Jean Michel (Editor)
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Springer, 1994. Paperback. New. reprint edition. 572 pages. 9.40x6.20x1.30 inches.
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