bohm vitense (16 Ergebnisse)

Zustand: Fair. Volume 1. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In fair condition, suitable as a study copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,500grams, ISBN:0521348692.

Zustand: Good. Volume 2. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft 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,650grams, ISBN:9780521348706.

paperback. Zustand: Very Good.

Zustand: Fair. Volume 2. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. Clean from markings. In fair condition, suitable as a study copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,650grams, ISBN:9780521348706.

Zustand: Fair. Volume 3. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. Clean from markings. In fair condition, suitable as a study copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,700grams, ISBN:9780521348713.

Zustand: Good. Volume 1. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. Clean from markings. 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,550grams, ISBN:0521348692.

Zustand: Good. Volume 2. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. Clean from markings. 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,550grams, ISBN:9780521348706.

Zustand: Fair. Volume 3. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. Clean from markings. In fair condition, suitable as a study copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,650grams, ISBN:9780521348713.

Softcover/Taschenbuch. Zustand: Sehr gut. kA. Auflage. Anzahl Bände: 1 - Bd.Nr.: kA - Sprache: en - Einband: Paperback - Gewicht: 320 - Illust.: - Zustand: Sehr gut - kaum Gebrauchsspuren.

Softcover/Taschenbuch. Zustand: Sehr gut. kA. Auflage. Anzahl Bände: 1 - Bd.Nr.: kA - Sprache: en - Einband: Paperback - Gewicht: 350 - Illust.: - Zustand: Sehr gut - leichte Gebrauchsspuren.

Zustand: New. In.

Zustand: New. This work conveys the basic physical ideas and laws used in the study of the outer layers of a star. It introduces stellar magnitudes, spectra and temperatures and includes a discussion of radiative transfer in a stellar atmosphere. The accessible structural components are also described. Num Pages: 264 pages, 15 half-tones, 119 diagrams, references, index. BIC Classification: PHVB. Category: (P) Professional & Vocational; (U) Tertiary Education (US: College). Dimension: 246 x 189 x 14. Weight in Grams: 492. . 2010. paperback. . . . . Books ship from the US and Ireland.

Broschur. Zustand: Wie neu. 245 Astrophysik Naturwissenschaften natural sciences Ex-Library. Fußschnitt leicht fleckig Additional cover foliation. Guter Zustand/ Good Ex-Library. Fußschnitt leicht fleckig ha1088078 Sprache: Englisch Gewicht in Gramm: 510.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This textbook introduces basic elements of fundamental astronomy and astrophysics which serve as a foundation for understanding the structure, evolution, and observed properties of stars. The first half of the book explains how stellar motions, distances, luminosities, colours, radii, masses and temperatures are measured or derived. The author then shows how data of these sorts can be arranged to classify stars through their spectra. Stellar rotation and stellar magnetic fields are introduced. Stars with peculiar spectra and pulsating stars also merit special attention. The endpoints of stellar volutions are briefly described. There is a separate chapter on the Sun and a final one on interstellar absorption. The usefulness of this text is enhanced by the inclusion of problems for students, tables of astronomical constants, and a selective bibliography.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book is the final one in a series of three texts which together provide a modern, complete and authoritative account of our present knowledge of the stars. It discusses the internal structure and the evolution of stars, and is completely self-contained. There is an emphasis on the basic physics governing stellar structure and the basic ideas on which our understanding of stellar structure is based. The book also provides a comprehensive discussion of stellar evolution. Careful comparison is made between theory and observation, and the author has thus provided a lucid and balanced introductory text for the student. As for volumes 1 and 2, volume 3 is self-contained and can be used as an independent textbook. The author has not only taught but has also published many original papers in this subject. Her clear and readable style should make this text a first choice for undergraduate and beginning graduate students taking courses in astronomy and particularly in stellar astrophysics.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This comprehensive textbook conveys the basic physical ideas and laws used in the study of the outer layers of a star. The stellar atmosphere emits the light which we see. The only layers of a star where we can get direct information about temperature, pressure and composition are in the atmosphere. This complete account first introduces stellar magnitudes, spectra and temperatures. This is followed by a full discussion of radiative transfer in a stellar atmosphere, which leads to descriptions of line formation, the spectrum of hydrogen, and spectral analysis. Finally the structural components that are accessible, such as the convestion zone, chromosphere, corona, and mass outflow are described. The book will interest any student with a knowledge of physics and mathematics who needs to learn about stellar atmospheres.