Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 120,17
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: California Books, Miami, FL, Estados Unidos de America
EUR 122,80
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 129,56
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 129,66
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 139,36
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Cambridge University Press CUP, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: Books Puddle, New York, NY, Estados Unidos de America
EUR 177,34
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Añadir al carritoCondición: New. pp. 912 Index.
EUR 132,48
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Añadir al carritoGebunden. Condición: 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 .
Librería: Revaluation Books, Exeter, Reino Unido
EUR 179,79
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Añadir al carritoHardcover. Condición: Brand New. 864 pages. 9.84x1.81x7.64 inches. In Stock.
Idioma: Inglés
Publicado por Cambridge University Press Jan 2013, 2013
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 183,17
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Añadir al carritoBuch. Condición: Neu. Neuware - Describes how stars respond to microscopic physics, from formation, through hydrogen-burning phases, up to the onset of helium burning.
Idioma: Inglés
Publicado por Cambridge University Press, Cambridge, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: Grand Eagle Retail, Bensenville, IL, Estados Unidos de America
EUR 122,51
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. Condición: 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.
Librería: Revaluation Books, Exeter, Reino Unido
EUR 123,71
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Añadir al carritoHardcover. Condición: Brand New. 864 pages. 9.84x1.81x7.64 inches. In Stock. This item is printed on demand.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: Majestic Books, Hounslow, Reino Unido
EUR 174,24
Cantidad disponible: 4 disponibles
Añadir al carritoCondición: New. Print on Demand pp. 912 313 Illus.
Idioma: Inglés
Publicado por Cambridge University Press, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: Biblios, Frankfurt am main, HESSE, Alemania
EUR 176,75
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Añadir al carritoCondición: New. PRINT ON DEMAND pp. 912.
Idioma: Inglés
Publicado por Cambridge University Press, Cambridge, 2012
ISBN 10: 1107016568 ISBN 13: 9781107016569
Librería: CitiRetail, Stevenage, Reino Unido
EUR 156,36
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. Condición: 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.