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Stellar Atmospheres: Beyond Classical Models - I. Hubeny#D. Hummer#L. Crivellari
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I. Hubeny#D. Hummer#L. Crivellari:

Stellar Atmospheres: Beyond Classical Models - nouveau livre

ISBN: 9780792313434

ID: 692758660

The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics; even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored. Proceedings of the NATO Advanced Research Workshop, Trieste, Italy, September 3-7, 1990 Bücher > Fremdsprachige Bücher > Englische Bücher gebundene Ausgabe 31.07.1991, Springer, .199

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Stellar Atmospheres: Beyond Classical Models - L. Crivellari
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L. Crivellari:

Stellar Atmospheres: Beyond Classical Models - nouveau livre

ISBN: 9780792313434

[ED: Buch], [PU: Springer], Neuware - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored. -, [SC: 0.00], Neuware, gewerbliches Angebot, 235x155x31 mm, [GW: 877g]

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Stellar Atmospheres: Beyond Classical Models - L. Crivellari
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L. Crivellari:
Stellar Atmospheres: Beyond Classical Models - nouveau livre

ISBN: 9780792313434

[ED: Buch], [PU: Springer], Neuware - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored., [SC: 0.00], Neuware, gewerbliches Angebot, 23.5x15.5x cm, [GW: 1870g]

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Stellar Atmospheres: Beyond Classical Models - L. Crivellari
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L. Crivellari:
Stellar Atmospheres: Beyond Classical Models - nouveau livre

ISBN: 9780792313434

[ED: Buch], [PU: Springer], Neuware - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored., [SC: 0.00], Neuware, gewerbliches Angebot, 23.5x15.5x cm, [GW: 1870g]

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Stellar Atmospheres: Beyond Classical Models - L. Crivellari
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L. Crivellari:
Stellar Atmospheres: Beyond Classical Models - nouveau livre

ISBN: 9780792313434

[ED: Buch], [PU: Springer], Neuware - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored., [SC: 2.00], Neuware, gewerbliches Angebot, 235x155x31 mm, [GW: 877g]

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Détails sur le livre
Stellar Atmospheres: Beyond Classical Models
Auteur:

L. Crivellari

Titre:

Stellar Atmospheres: Beyond Classical Models

ISBN:

0792313437

Informations détaillées sur le livre - Stellar Atmospheres: Beyond Classical Models


EAN (ISBN-13): 9780792313434
ISBN (ISBN-10): 0792313437
Version reliée
Date de parution: 1991
Editeur: Springer-Verlag GmbH
480 Pages
Poids: 0,877 kg
Langue: eng/Englisch

Livre dans la base de données depuis 26.03.2007 17:10:31
Livre trouvé récemment le 18.11.2016 12:38:58
ISBN/EAN: 0792313437

ISBN - Autres types d'écriture:
0-7923-1343-7, 978-0-7923-1343-4

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