Luis balona (22 resultados)

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Librería: Anybook.com, Lincoln, Reino UnidoAnybook.com
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EUR 34,52
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Condición: Good. Volume 305. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,800grams, ISBN:9781583811542.

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Librería: Ria Christie Collections, Uxbridge, Reino UnidoRia Christie Collections
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EUR 60,65
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Condición: New. In.

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Librería: Chiron Media, Wallingford, , Reino UnidoChiron Media
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EUR 57,37
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Paperback. Condición: New.

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Librería: Le-Livre, SABLONS, , FranciaLe-Livre
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EUR 35,80
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Couverture rigide. Condición: bon. R260269814: 1994. In-8. Relié. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 550 pages augmentées de quelques figures en noir et blanc dans texte. Avec Jaquette. . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Pulsation, Rotation and Mass Loss in Early-Type Stars
. Ed(s): Balona, Luis A.; Henrichs, Huib F.; Le Contel, Jean Michel
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Librería: Kennys Bookshop and Art Galleries Ltd., Galway, GY, IrlandaKennys Bookshop and Art Galleries Ltd.
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EUR 72,12
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Condición: New. In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together in order to broaden our understanding of O and B stars. Editor(s): Balona, Luis A.; Henrichs, Huib F.; Le Contel, Jean Michel. Series: International Astronomical Union Symposia (Closed). Num…Pages: 550 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 240 x 160 x 30. Weight in Grams: 1031. . 1994. Softcover reprint of the original 1st ed. 1994. Paperback. . . . .

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Librería: Books Puddle, New York, NY, Estados Unidos de AmericaBooks Puddle
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EUR 85,57
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Condición: New. pp. 572.
Idioma: Inglés
Editorial: San Francisco, Astronomical Society of the Pacific, 2003
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- Primera edición
Librería: Buch & Cafe Antiquarius, Bonn, NRW, AlemaniaBuch & Cafe Antiquarius
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EUR 49,00
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Gr.-8°, original hardcover. 1. ed. With numerous images, XVII, 413 p. Shelfmark on spine, stamp on Title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Pulsation, Rotation and Mass Loss in Early-Type Stars
. Ed(s): Balona, Luis A.; Henrichs, Huib F.; Le Contel, Jean Michel
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Librería: Kennys Bookstore, Olney, MD, Estados Unidos de AmericaKennys Bookstore
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EUR 90,67
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Condición: New. In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together in order to broaden our understanding of O and B stars. Editor(s): Balona, Luis A.; Henrichs, Huib F.; Le Contel, Jean Michel. Series: International Astronomical Union Symposia (Closed). Num…Pages: 550 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 240 x 160 x 30. Weight in Grams: 1031. . 1994. Softcover reprint of the original 1st ed. 1994. Paperback. . . . . Books ship from the US and Ireland.

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
Balona, Luis A. (Editor) / Henrichs, Huib F. (Editor) / Le Contel, Jean Michel (Editor)
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Librería: Revaluation Books, Exeter, , Reino UnidoRevaluation Books
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EUR 84,37
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Paperback. Condición: Brand New. reprint edition. 572 pages. 9.40x6.20x1.30 inches. In Stock.

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Librería: Ria Christie Collections, Uxbridge, Reino UnidoRia Christie Collections
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EUR 93,68
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Condición: New. In.

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Librería: preigu, Osnabrück, Alemaniapreigu
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EUR 50,25
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Taschenbuch. Condición: Neu. 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 | Luis A. Balona (u. a.) | Taschenbuch | xxii | Englisch | 1994 | Springer | EAN 9780792330455 | Verantwortliche… Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

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Librería: AHA-BUCH GmbH, Einbeck, AlemaniaAHA-BUCH GmbH
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EUR 59,97
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Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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 ty…pes 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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Librería: moluna, Greven, , Alemaniamoluna
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EUR 104,18
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Gebunden. Condición: 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. Thanks to advances in digital spectroscopy, new types of pu.

Pulsation, Rotation and Mass Loss in Early-Type Stars
Balona, Luis A./ Henrichs, Huib F./ Le Contel, Jean Michel (Editor)
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Librería: Revaluation Books, Exeter, , Reino UnidoRevaluation Books
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EUR 146,56
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Hardcover. Condición: Brand New. 576 pages. 9.75x6.75x1.25 inches. In Stock.

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Librería: AHA-BUCH GmbH, Einbeck, AlemaniaAHA-BUCH GmbH
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EUR 193,80
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Buch. Condición: Neu. Neuware - 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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Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, , AlemaniaBuchWeltWeit Ludwig Meier e.K.
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EUR 53,49
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Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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 spec…troscopy, 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. 576 pp. Englisch.

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Librería: Majestic Books, Hounslow, , Reino UnidoMajestic Books
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EUR 83,37
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Condición: New. Print on Demand pp. 572 21 Illus.

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Librería: THE SAINT BOOKSTORE, Southport, , Reino UnidoTHE SAINT BOOKSTORE
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EUR 71,68
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Paperback / softback. Condición: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.

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Librería: Biblios, frankfurt am main, HESSE, AlemaniaBiblios
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EUR 83,86
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Condición: New. PRINT ON DEMAND pp. 572.

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Librería: moluna, Greven, , Alemaniamoluna
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EUR 48,37
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Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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.

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Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemaniabuchversandmimpf2000
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EUR 53,49
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Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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 spectros…copy, 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.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 576 pp. Englisch.

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Librería: THE SAINT BOOKSTORE, Southport, , Reino UnidoTHE SAINT BOOKSTORE
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Hardback. Condición: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.