Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: GreatBookPrices, Columbia, MD, U.S.A.
EUR 120,17
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Aggiungi al carrelloCondizione: New.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: California Books, Miami, FL, U.S.A.
EUR 122,80
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Aggiungi al carrelloCondizione: New.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: GreatBookPrices, Columbia, MD, U.S.A.
EUR 129,56
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Aggiungi al carrelloCondizione: As New. Unread book in perfect condition.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: GreatBookPricesUK, Woodford Green, Regno Unito
EUR 129,66
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Aggiungi al carrelloCondizione: New.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: GreatBookPricesUK, Woodford Green, Regno Unito
EUR 139,36
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Aggiungi al carrelloCondizione: As New. Unread book in perfect condition.
Lingua: Inglese
Editore: Cambridge University Press CUP, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: Books Puddle, New York, NY, U.S.A.
Condizione: New. pp. 912 Index.
EUR 132,48
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Aggiungi al carrelloGebunden. Condizione: 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 .
Da: Revaluation Books, Exeter, Regno Unito
EUR 179,79
Quantità: 2 disponibili
Aggiungi al carrelloHardcover. Condizione: Brand New. 864 pages. 9.84x1.81x7.64 inches. In Stock.
Lingua: Inglese
Editore: Cambridge University Press Jan 2013, 2013
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 183,17
Quantità: 2 disponibili
Aggiungi al carrelloBuch. Condizione: Neu. Neuware - Describes how stars respond to microscopic physics, from formation, through hydrogen-burning phases, up to the onset of helium burning.
Lingua: Inglese
Editore: Cambridge University Press, Cambridge, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: Grand Eagle Retail, Bensenville, IL, U.S.A.
Hardcover. Condizione: new. Hardcover. 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. 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 prepare beginning graduate students and senior undergraduates to program and calculate evolutionary models. This item is printed on demand. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
Da: Revaluation Books, Exeter, Regno Unito
EUR 123,71
Quantità: 1 disponibili
Aggiungi al carrelloHardcover. Condizione: Brand New. 864 pages. 9.84x1.81x7.64 inches. In Stock. This item is printed on demand.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: Majestic Books, Hounslow, Regno Unito
EUR 174,24
Quantità: 4 disponibili
Aggiungi al carrelloCondizione: New. Print on Demand pp. 912 313 Illus.
Lingua: Inglese
Editore: Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: Biblios, Frankfurt am main, HESSE, Germania
EUR 176,75
Quantità: 4 disponibili
Aggiungi al carrelloCondizione: New. PRINT ON DEMAND pp. 912.
Lingua: Inglese
Editore: Cambridge University Press, Cambridge, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Da: CitiRetail, Stevenage, Regno Unito
EUR 156,36
Quantità: 1 disponibili
Aggiungi al carrelloHardcover. Condizione: new. Hardcover. 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. 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 prepare beginning graduate students and senior undergraduates to program and calculate evolutionary models. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.