1. Angular Momentum and Mass Loss for Hot Stars: 316 (Nato Science Series C:, 316)
Price: USD 11.39
Dealer: ZVAB, HALCYON BOOKS
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer] Hardcover ALL ITEMS ARE DISPATCHED FROM THE UK WITHIN 48 HOURS ( BOOKS ORDERED OVER THE WEEKEND DISPATCHED ON MONDAY) ALL OVERSEAS ORDERS SENT BY TRACKABLE AIR MAIL. IF YOU ARE LOCATED OUTSIDE THE UK PLEASE ASK US FOR A POSTAGE QUOTE FOR MULTI VOLUME SETS BEFORE ORDERING [LONDON, United Kingdom] [Publication Year: 1990]  

2. Angular Momentum and Mass Loss for Hot Stars: 316 (Nato Science Series C:, 316)
Price: USD 12.21
Dealer: AbebooksUK, HALCYON BOOKS
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer] Hardcover ALL ITEMS ARE DISPATCHED FROM THE UK WITHIN 48 HOURS ( BOOKS ORDERED OVER THE WEEKEND DISPATCHED ON MONDAY) ALL OVERSEAS ORDERS SENT BY TRACKABLE AIR MAIL. IF YOU ARE LOCATED OUTSIDE THE UK PLEASE ASK US FOR A POSTAGE QUOTE FOR MULTI VOLUME SETS BEFORE ORDERING [LONDON, United Kingdom] [Publication Year: 1990]  

3. Angular Momentum and Mass Loss for Hot Stars: 316 Nato Science Series C: 316
Price: USD 15.54
Dealer: Biblio, HALCYON BOOKS
Description: Springer, Date: 1990-08-31. Hardcover. Very Good. 2.7979 in x 24.1816 in x 16.3875 in. 1990. Springer ISBN 0792308816 9780792308812 [GB] 

4. Angular Momentum and Mass Loss for Hot Stars Nato Science Series C:, 316
by Willson, L.A. and R. Stalio: 
Price: USD 19.45
Dealer: ZVAB, books4less (Versandantiquariat Petra Gros GmbH & Co. KG)
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer Verlag;] Hardcover 365 Seiten; Der Erhaltungszustand des hier angebotenen Werks ist trotz seiner Bibliotheksnutzung sehr sauber. Es befindet sich neben dem Rückenschild lediglich ein Bibliotheksstempel im Buch; ordnungsgemäß entwidmet. Sprache: Englisch Gewicht in Gramm: 833 [Welling, Germany] [Publication Year: 1990]  

5. Angular Momentum and Mass Loss for Hot Stars Nato Science Series C:, 316
by Willson, L.A. and R. Stalio: 
Price: USD 21.46
Dealer: AbebooksDE, books4less (Versandantiquariat Petra Gros GmbH & Co. KG)
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer Verlag;] Hardcover 365 Seiten; Der Erhaltungszustand des hier angebotenen Werks ist trotz seiner Bibliotheksnutzung sehr sauber. Es befindet sich neben dem Rückenschild lediglich ein Bibliotheksstempel im Buch; ordnungsgemäß entwidmet. Sprache: Englisch Gewicht in Gramm: 833 [Welling, Germany] [Publication Year: 1990]  

6. Angular Momentum and Mass Loss for Hot Stars: 316 (Nato Science Series C: , 316)
by Willson, L a (Editor), and Stalio, R (Editor) 
Price: USD 22.26
Dealer: Alibris, Halcyon Books via Alibris
Description: Springer 1990 1990 ed. Hardcover Very good ALL ITEMS ARE SENT BY ROYAL MAIL. 

7. Angular Momentum and Mass Loss for Hot Stars
by Willson, L a (Editor), and Stalio, R (Editor) 
Price: USD 206.66
Dealer: Alibris
Description: Dordrecht Springer 1990 1990 ed. Hard cover New. Sewn binding. Cloth over boards. 365 p. NATO Science Series C:, 316. 

8. Angular Momentum and Mass Loss for Hot Stars (Nato Science Series C:) [Hardcover ]
Price: USD 214.97
Dealer: Abebooks, booksXpress
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer] Hardcover [Bayonne, NJ, U.S.A.] [Publication Year: 1990]  

9. Angular Momentum and Mass Loss for Hot Stars
by R. Stalio 
Price: USD 222.65
Dealer: ZVAB, AHA-BUCH GmbH
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer Netherlands] Hardcover Druck auf Anfrage Neuware - Printed after ordering - Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, the mass loss rates, and the rotation velocity. If the same mechanisms are able to drive mass loss from the main sequence A stars, as has recently been proposed, then the current interpretations of a number of observations will be drastically affected: e. g. the ages of clusters may be incorrect by up to a factor of two, and the surface abundances of isotopes of He, Li and Be may no longer give constraints on cosmological nucleosynthesis. There are also effects on the evolution of the abundances of elements in the interstellar medium and on the general evolution of populations of stars. Thus the questions of the mechanisms of angular momentum and mass loss of stars more massive than the sun is important not only for stellar studies but for the foundations of much of modern astrophysics. [Einbeck, Germany] [Publication Year: 1990]  

10. Angular Momentum and Mass Loss for Hot Stars (Nato Science Series C:, 316)
Price: USD 230.44
Dealer: Abebooks, Lucky's Textbooks
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer] Hardcover [Dallas, TX, U.S.A.] [Publication Year: 1990]  

11. Angular Momentum and Mass Loss for Hot Stars
by R. Stalio 
Price: USD 245.72
Dealer: AbebooksDE, AHA-BUCH GmbH
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer Netherlands] Hardcover Druck auf Anfrage Neuware - Printed after ordering - Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, the mass loss rates, and the rotation velocity. If the same mechanisms are able to drive mass loss from the main sequence A stars, as has recently been proposed, then the current interpretations of a number of observations will be drastically affected: e. g. the ages of clusters may be incorrect by up to a factor of two, and the surface abundances of isotopes of He, Li and Be may no longer give constraints on cosmological nucleosynthesis. There are also effects on the evolution of the abundances of elements in the interstellar medium and on the general evolution of populations of stars. Thus the questions of the mechanisms of angular momentum and mass loss of stars more massive than the sun is important not only for stellar studies but for the foundations of much of modern astrophysics. [Einbeck, Germany] [Publication Year: 1990]  

12. Angular Momentum and Mass Loss for Hot Stars
by LA. Willson L. A. 
Price: USD 252.60
Dealer: Biblio, Ria Christie Collections
Description: Hard Cover. New. New Book; Fast Shipping from UK; Not signed; Not First Edition; The Angular Momentum and Mass Loss for Hot Stars. ISBN 0792308816 9780792308812 [GB] 

13. Angular Momentum and Mass Loss for Hot Stars Nato Science Series C:
by Willson LA. Editor; Stalio R. Editor; L. A. 
Price: USD 287.00
Dealer: Biblio, SOUTHAUSTRALIANBOOKS
Description: Springer. Hardcover. New. 9x6x1. Springer ISBN 0792308816 9780792308812 [US] 

14. Angular Momentum and Mass Loss for Hot Stars (Nato Science Series C: (316))
Price: USD 351.57
Dealer: AbebooksUK, dsmbooks
Description: ISBN10: 0792308816, ISBN13: 9780792308812, [publisher: Springer] Hardcover Like New [liverpool, United Kingdom] [Publication Year: 1990]