Stellar Atmospheres: Beyond Classical Models:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1991
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
341 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | 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 |
| Beschreibung: | 1 Online-Ressource (XIV, 461 p) |
| ISBN: | 9789401135542 9789401055741 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-011-3554-2 |
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Datensatz im Suchindex
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| discipline | Physik |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:58Z |
| institution | BVB |
| isbn | 9789401135542 9789401055741 |
| issn | 1389-2185 |
| language | English |
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| spelling | Crivellari, L. Verfasser aut Stellar Atmospheres: Beyond Classical Models edited by L. Crivellari, I. Hubeny, D. G. Hummer Proceedings of the NATO Advanced Research Workshop, Trieste, Italy, September 3-7, 1990 Dordrecht Springer Netherlands 1991 1 Online-Ressource (XIV, 461 p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 341 1389-2185 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 Physics Astrophysics and Astroparticles Hubeny, I. Sonstige oth Hummer, D. G. Sonstige oth https://doi.org/10.1007/978-94-011-3554-2 Verlag Volltext |
| spellingShingle | Crivellari, L. Stellar Atmospheres: Beyond Classical Models Physics Astrophysics and Astroparticles |
| title | Stellar Atmospheres: Beyond Classical Models |
| title_alt | Proceedings of the NATO Advanced Research Workshop, Trieste, Italy, September 3-7, 1990 |
| title_auth | Stellar Atmospheres: Beyond Classical Models |
| title_exact_search | Stellar Atmospheres: Beyond Classical Models |
| title_full | Stellar Atmospheres: Beyond Classical Models edited by L. Crivellari, I. Hubeny, D. G. Hummer |
| title_fullStr | Stellar Atmospheres: Beyond Classical Models edited by L. Crivellari, I. Hubeny, D. G. Hummer |
| title_full_unstemmed | Stellar Atmospheres: Beyond Classical Models edited by L. Crivellari, I. Hubeny, D. G. Hummer |
| title_short | Stellar Atmospheres: Beyond Classical Models |
| title_sort | stellar atmospheres beyond classical models |
| topic | Physics Astrophysics and Astroparticles |
| topic_facet | Physics Astrophysics and Astroparticles |
| url | https://doi.org/10.1007/978-94-011-3554-2 |
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