Idioma: Inglés
Publicado por Kluwer Academic Publishers (KAP), Boston, Dordrecht, London, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
Librería: CURIO, Cleethorpes, North East Lincolnshire, Reino Unido
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Añadir al carritoHardcover. Condición: Very Good. No Jacket. Hardback copy, no dustjacket as issued. 428pp. Charts and graphs throughout. Not library copy, no inscriptions. (45/4).
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Librería: Ria Christie Collections, Uxbridge, Reino Unido
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Librería: Books Puddle, New York, NY, Estados Unidos de America
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Añadir al carritoCondición: New. pp. xii + 431.
Librería: Books Puddle, New York, NY, Estados Unidos de America
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Añadir al carritoCondición: New. pp. 448.
Idioma: Inglés
Publicado por Springer Netherlands, Springer Netherlands, 2012
ISBN 10: 9401060223 ISBN 13: 9789401060226
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 244,86
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Añadir al carritoTaschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observa tional, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and estab lish both models and atomic data, and eventually led to the now accepted, so-called 'absolute' abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei.
Idioma: Inglés
Publicado por Springer Netherlands, Springer Netherlands, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 244,86
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Añadir al carritoBuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observa tional, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and estab lish both models and atomic data, and eventually led to the now accepted, so-called 'absolute' abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei.
Librería: Mispah books, Redhill, SURRE, Reino Unido
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Añadir al carritoPaperback. Condición: Like New. Like New. book.
Librería: Revaluation Books, Exeter, Reino Unido
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Añadir al carritoPaperback. Condición: Brand New. reprint edition. 428 pages. 9.50x6.25x1.25 inches. In Stock.
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Añadir al carritoHardcover. Condición: Brand New. 444 pages. 9.50x6.50x1.00 inches. In Stock.
Librería: Mispah books, Redhill, SURRE, Reino Unido
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Añadir al carritoHardcover. Condición: Like New. Like New. book.
Librería: BUCHSERVICE / ANTIQUARIAT Lars Lutzer, Wahlstedt, Alemania
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Añadir al carritoHardcover. Condición: gut. 1998. Solar Composition and its Evolution from Core to Corona : Proceedings of an ISSI Workshop 2630 January 1998, Bern, Switzerland In deutscher Sprache. pages.
Librería: suspiratio - online bücherstube lic.phil h.b., Basel, Suiza
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Añadir al carritoHardcover. Condición: Sehr gut. sehr gut, near FINE - lager nur a-916 Language: DEU.
Librería: Brook Bookstore On Demand, Napoli, NA, Italia
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Añadir al carritoCondición: new. Questo è un articolo print on demand.
Librería: moluna, Greven, Alemania
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Añadir al carritoCondición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscip.
Librería: moluna, Greven, Alemania
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Añadir al carritoGebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscip.
Idioma: Inglés
Publicado por Springer Netherlands, Springer Netherlands Dez 1998, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
EUR 235,39
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Añadir al carritoBuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observa tional, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and estab lish both models and atomic data, and eventually led to the now accepted, so-called 'absolute' abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei. 448 pp. Englisch.
Idioma: Inglés
Publicado por Springer Netherlands, Springer Netherlands Okt 2012, 2012
ISBN 10: 9401060223 ISBN 13: 9789401060226
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
EUR 235,39
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Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observa tional, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and estab lish both models and atomic data, and eventually led to the now accepted, so-called 'absolute' abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 448 pp. Englisch.
Librería: Majestic Books, Hounslow, Reino Unido
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Añadir al carritoCondición: New. Print on Demand pp. xii + 431.
Librería: Majestic Books, Hounslow, Reino Unido
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Añadir al carritoCondición: New. Print on Demand pp. 448.
Librería: Biblios, Frankfurt am main, HESSE, Alemania
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Añadir al carritoCondición: New. PRINT ON DEMAND pp. xii + 431.
Librería: Biblios, Frankfurt am main, HESSE, Alemania
EUR 321,92
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Añadir al carritoCondición: New. PRINT ON DEMAND pp. 448.