Language: English
Published by Dordrecht, D. Reidel Publishing Company, 1979
ISBN 10: 9027709890 ISBN 13: 9789027709899
Seller: ABC Versand e.K., Aarbergen, Germany
Condition: Gut. 501 Seiten mit Gebrauchsspuren, Bibliotheksexemplar der Sternwarte des Physikalischen Vereins Frankfurt/Main, Umschlag, Schnitt und Seiten nachgedunkelt, Umschlag, Ecken und Kanten leicht berieben, innen sauber und ordentlich Q71 Sprache: Englisch Gewicht in Gramm: 1001 24,4 x 17,0 x 3,0 cm, Softcover/Paperback.
Hardcover. Condition: Good. Slight wear on dustcover, Book as new. English.
501 S. mit zahlreichen Abbildungen, 9027709890 Sprache: Englisch Gewicht in Gramm: 950 Groß 8°, Original-Karton (Softcover), Ecken minimal bestoßen, Vortitel mit kleinem Namensstempel, insgesamt gutes und innen sauberes Exemplar,
Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Condition: New. pp. 526.
Language: English
Published by Springer Netherlands, 1979
ISBN 10: 9027709890 ISBN 13: 9789027709899
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Condition: New.
Seller: Revaluation Books, Exeter, United Kingdom
Paperback. Condition: Brand New. reprint edition. 520 pages. 9.61x6.69x1.19 inches. In Stock.
Language: English
Published by D. Reidel publishing company, 1979
ISBN 10: 9027709882 ISBN 13: 9789027709882
Couverture rigide. Condition: bon. R260269756: 1979. In-8. Relié. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 501 pages. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.
Language: English
Published by Springer Netherlands, Springer, 1979
ISBN 10: 9027709890 ISBN 13: 9789027709899
Seller: AHA-BUCH GmbH, Einbeck, Germany
Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial 'rounding up' of the Scienti fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup' which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per tains to the O-type stars.
Seller: Mispah books, Redhill, SURRE, United Kingdom
Paperback. Condition: Very Good. Dust Jacket may NOT BE INCLUDED.CDs may be missing. SHIPS FROM MULTIPLE LOCATIONS. book.
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Paperback/ broschiert. Condition: Gut. 501 S. Guter Zustand ha1075923 Sprache: Englisch Gewicht in Gramm: 1050.
Condition: gut. 1979. Mass Loss and Evolution of O-Type Star. (= International Astronomical Union - Symposium No. 83). In deutscher Sprache. pages.
Language: English
Published by Springer Netherlands, Springer Netherlands Mai 1979, 1979
ISBN 10: 9027709890 ISBN 13: 9789027709899
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany
Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial 'rounding up' of the Scienti fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup' which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per tains to the O-type stars. 524 pp. Englisch.
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Condition: New. Print on Demand pp. 526 67:B&W 6.69 x 9.61 in or 244 x 170 mm (Pinched Crown) Perfect Bound on White w/Gloss Lam.
Seller: Biblios, Frankfurt am main, HESSE, Germany
Condition: New. PRINT ON DEMAND pp. 526.
Language: English
Published by Springer Netherlands, Springer Mai 1979, 1979
ISBN 10: 9027709890 ISBN 13: 9789027709899
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial 'rounding up' of the Scienti fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup' which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per tains to the O-type stars.Springer-Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 524 pp. Englisch.
Seller: preigu, Osnabrück, Germany
Taschenbuch. Condition: Neu. Mass Loss and Evolution of O-Type Stars | P. S. Conti (u. a.) | Taschenbuch | International Astronomical Union Symposia | 520 S. | Englisch | 1979 | Springer | EAN 9789027709899 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on Demand.