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Published by Springer, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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Published by Springer Nature Singapore Feb 2004, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The rsteditionofthistextappearedin1994.Shortlyafterthethirdprinting, our editor suggested that we attempt a second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of, etc.) our new coauth- colleague Virginia Trimble to join us. (Welcome Virginia!) We (i.e., all three of us) hope that you agree that the present edition is a great improvement compared to the 1994 e ort. Our objectives in this edition are the same ones we set forth in 1994: Whatyouwill ndisatextdesignedforourtargetaudience:thety- cal senior undergraduate or beginning graduate student in astronomy or astrophysics who wishes an overview of stellar structure and e- lution with just enough detail to understand the general picture. She or he can go on from there to more specialized texts or directly to the research literature depending on talent and interests. To this end, this text presents the basic physical principles without chasing all the (interesting!) details. For those of you familiar with the rst edition, you will nd that some things have not been changed substantially (F = ma is still F = ma), while othersde nitelyhave.Forexample,Chapter2hasbeencompletelyrewritten. 526 pp. Englisch.
Published by Springer Nature Singapore Feb 2004, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The rsteditionofthistextappearedin1994.Shortlyafterthethirdprinting, our editor suggested that we attempt a second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of, etc.) our new coauth- colleague Virginia Trimble to join us. (Welcome Virginia!) We (i.e., all three of us) hope that you agree that the present edition is a great improvement compared to the 1994 e ort. Our objectives in this edition are the same ones we set forth in 1994: Whatyouwill ndisatextdesignedforourtargetaudience:thety- cal senior undergraduate or beginning graduate student in astronomy or astrophysics who wishes an overview of stellar structure and e- lution with just enough detail to understand the general picture. She or he can go on from there to more specialized texts or directly to the research literature depending on talent and interests. To this end, this text presents the basic physical principles without chasing all the (interesting!) details. For those of you familiar with the rst edition, you will nd that some things have not been changed substantially (F = ma is still F = ma), while othersde nitelyhave.Forexample,Chapter2hasbeencompletelyrewritten. 526 pp. Englisch.
Published by Springer, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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Published by Springer, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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Published by Springer New York Feb 2004, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The rsteditionofthistextappearedin1994.Shortlyafterthethirdprinting , our editor suggested that we attempt a second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of, etc.) our new coauth- colleague Virginia Trimble to join us. (Welcome Virginia!) We (i.e., all three of us) hope that you agree that the present edition is a great improvement compared to the 1994 e ort. Our objectives in this edition are the same ones we set forth in 1994: Whatyouwill ndisatextdesignedforourtargetaudience:thety- cal senior undergraduate or beginning graduate student in astronomy or astrophysics who wishes an overview of stellar structure and e- lution with just enough detail to understand the general picture. She or he can go on from there to more specialized texts or directly to the research literature depending on talent and interests. To this end, this text presents the basic physical principles without chasing all the (interesting!) details. For those of you familiar with the rst edition, you will nd that some things have not been changed substantially (F = ma is still F = ma), while othersde nitelyhave.Forexample,Chapter2hasbeencompletelyrewritten.
Published by Springer, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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ISBN 10: 0387200894ISBN 13: 9780387200897
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Published by Springer Verlag, 2004
ISBN 10: 0387200894ISBN 13: 9780387200897
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