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hardcover. Zustand: Good. Cover and edges may have some wear.

hardcover. Zustand: Very Good. Cover and edges may have some wear.

Hardcover. Zustand: Like New. First Edition. A firm and square hardback with sharp corners and strong joints, just showing a few very minor cosmetic rubs. Hence a non-text page has a small 'damaged' stamp. Despite such this book is actually in nearly new condition and appears unread. Thus the contents are crisp, fresh and tight; no pen-marks. Now offered for sale at a very sensible price.…

Gr.-8°, original hardcover. 1. ed. XV, 488 p. English Edition. Shelfmark, stamp on title and preliminary page, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Original Cloth - Hardcover. Zustand: Good Condition. No Dustjacket. First Edition. XV, 488 pages with figures; little signs of use, 6 pages with underlinings - good condition; 1,5 kg shipping weight.

Gebunden. Zustand: New. This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. The volume contains many illustrations and detailed numerical solutions to .

Hardcover. Zustand: Brand New. 600 pages. 9.80x1.30x7.50 inches. In Stock.

Hardcover. Zustand: Brand New. 864 pages. 9.84x1.81x7.64 inches. In Stock.

Buch. Zustand: Neu. Neuware - This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models.…