Mass loss evolution o type (19 résultats)

Etat : 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.…

Etat : As New. Unread book in perfect condition.

Hardcover. Etat : 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.

Etat : New.

Etat : New. In English.

Taschenbuch. Etat : 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.…

Etat : New. pp. 526.

Etat : New.

Paperback. Etat : Brand New. reprint edition. 520 pages. 9.61x6.69x1.19 inches. In Stock.

Couverture rigide. Etat : bon. R260269756: 1979. In-8. Relié. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 501 pages. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Paperback. Etat : Very Good. Dust Jacket may NOT BE INCLUDED.CDs may be missing. SHIPS FROM MULTIPLE LOCATIONS. book.

Paperback/ broschiert. Etat : Gut. 501 S. Guter Zustand ha1075923 Sprache: Englisch Gewicht in Gramm: 1050.

Etat : gut. 1979. Mass Loss and Evolution of O-Type Star. (= International Astronomical Union - Symposium No. 83). In deutscher Sprache. pages.

hardcover. Etat : Good. exlibrary hardcover book no dust jacket, usual library marks, has some light reader wear.

Taschenbuch. Etat : 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.…

Etat : 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.

Etat : New. PRINT ON DEMAND pp. 526.

Taschenbuch. Etat : 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.…