W d heintz (55 resultados)

SpiralBound. Condición: Very Good. Second Edition Pages 308, M1-16, Supplement S1-19, Appendix A1-98.

SpiralBound. Condición: Very Good. Second Edition Pages 308, M1-16, Supplement S1-19, Appendix A1-98.

Condición: very_good. Gently read. May have name of previous ownership, or ex-library edition. Binding tight; spine straight and smooth, with no creasing; covers clean and crisp. Minimal signs of handling or shelving. 100% GUARANTEE! Shipped with delivery confirmation, if you're not satisfied with purchase please return item! Ships USPS Media Mail.…

No Binding. Condición: Good. ORIGINAL reprint/offprint/Sonderdruck of journal article; no covers; small chips along gutter where disbound from larger publication; o/w in good condition. Journal.

No Binding. Condición: Good. ORIGINAL reprint/offprint/Sonderdruck of journal article; no covers; ex-astronomical observatory library; small chips along gutter where disbound from larger publication; o/w in good condition. Journal.

No Binding. Condición: Good. ORIGINAL reprint/offprint/Sonderdruck of journal article; no covers; small chips along gutter where disbound from larger publication; small tear on lower corner of last leaf; spine reinforced w/ tape; o/w in good condition. Journal.

Condición: Poor. Volume 15. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In poor condition, suitable as a reading copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,400grams, ISBN:902770886X. …

Perfect Paperback. Condición: Good. Clean text. Shelving code RF.

Condición: Good. Volume 15. 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. Re-bound by library. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,550grams, ISBN:902770886X.…

Condición: As New. Unread book in perfect condition.

Condición: As New. Unread book in perfect condition.

Condición: New.

Condición: New.

Paperback. Condición: Good. Clean text. Shelving code RF.

Condición: New. pp. xxi + 362.

Paperback. Condición: Brand New. 340 pages. 9.61x6.69x0.72 inches. In Stock.

Perfect Paperback. Condición: Brand New. 1st edition. 383 pages. 9.70x7.00x0.70 inches. In Stock.

Condición: New.

Softcover. Condición: sehr gut. Originalbroschur, 4°. 23-34 Seiten, ausgeschiedenes Bibliotheksexemplar, sehr gutes Exemplar. Veröfffentlichungen der Sternwarte München, Band 5, Nr. 2. Abdruck aus den Astronomischen Nachrichten. in deutscher Sprache.

Softcover. Condición: sehr gut. Originalbroschur, 4°. 49 Seiten, ausgeschiedenes Bibliotheksexemplar, sehr gutes Exemplar. Veröfffentlichungen der Sternwarte München, Band 5, Nr. 15. in deutscher Sprache.

Softcover. Originalbroschur. 4°. 315-339 SS. mit Tabellen und mehrseitigen Zahlentafeln. ausgeschiedenes Bibliotheksexemplar. Einband mit leichten Knickspuren. leicht berieben. sehr guter Zustand. The Astrophysical Journal, Supplement Series, Supplement Number 288, Vol. 29. Reprint: Sproul-Observatory, Nr. 244. in englischer Sprache (in english). …

Softcover. Condición: sehr gut. ein Blatt 4°. S. 787. mit 1 Tabelle. ausgeschiedenes Bibliotheksexemplar. etwas gebräunt. sehr guter Zustand. Reprinted from The Astrophysical Journal", 200 : 787. Reprint: Sproul-Observatory, Nr. 249. in englischer Sprache (in english).

Softcover. Originalbroschur, 4°. 85-88 Seiten, m. 2 Abb. Exemplar mit Querknick. etwas gebräunt. wenige Gebrauchsspuren. sehr gutes Ex. Abdruck aus Astronomische Nachrichten" Bd. 282, Heft 2. Veröffentlichungen der Sternwarte München Bd. 4, Nr. 13. in deutscher Sprache.

Softcover. Condición: sehr gut. Originalbroschur, 4°. 77-79 Seiten, ausgeschiedenes Bibliotheksexemplar, sehr gutes Exemplar. Veröfffentlichungen der Sternwarte München, Band 5, Nr. 8. Abdruck aus den Astronomischen Nachrichten. in deutscher Sprache.

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

Condición: Good. Volume 15. 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. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,550grams, ISBN:9027708851. …

Condición: New. pp. 188.

Condición: New. pp. 192.

Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: The patterns of evolution involving mass transfer appear to lead ultimately to single objects.…

Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: The patterns of evolution involving mass transfer appear to lead ultimately to single objects.…