Physics of Thermal Gaseous Nebulae: Physical Processes in Gaseous Nebulae
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1984
|
| Schriftenreihe: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
112 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Gaseous nebulae offer outstanding opportunities to atomic physicists, spectroscopists, plasma experts, and to observers and theoreticians alike for the study of attenuated ionized gases. These nebulae are often dusty, heated by radiation fields and by shocks. They are short-lived phenomena on the scale of a stellar lifetime, but their chemical compositions and internal kinematics may give important clues to advanced stages of stellar evolution. The material herein presented is based on lectures given at the University of Michigan, University of Queensland, University of California, Los Angeles, and in more abbreviated form at the Raman Institute, at the Scuola Internazionale di Trieste, and elsewhere. Much of it is derived origionally from the series "Physical Processes in Gaseous Nebulae" initiated at the Harvard College Observatory in the late 1930s. I have tried to emphasize the basic physics of the mechanisms involved and mention some of the uncertainties that underlie calculations of many basic parameters. Emphasis is placed on ionized plasmas with electron temperatures typically in the neighborhood of 10,OOOoK. Dust and other ingredients of the cold component of the interstellar medium are treated briefly from the point of view of their relation to hot plasmas of H II regions and planetaries. Chemical composition determinations for nebulae are discussed in some detail while the last section deals with interpretations of elemental abundances in the framework of stellar evolution and nucleogenesis. Gaseous nebulae offer some particularly engaging opportunities for studies of stellar evolution |
| Beschreibung: | 1 Online-Ressource (350p) |
| ISBN: | 9789401096393 9789027725462 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-010-9639-3 |
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Datensatz im Suchindex
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| author | Aller, Lawrence Hugh 1913-2003 |
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| author_sort | Aller, Lawrence Hugh 1913-2003 |
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| building | Verbundindex |
| bvnumber | BV042415708 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)906712762 (DE-599)BVBBV042415708 |
| dewey-full | 520 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
| dewey-raw | 520 |
| dewey-search | 520 |
| dewey-sort | 3520 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-010-9639-3 |
| format | Electronic eBook |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:58Z |
| institution | BVB |
| isbn | 9789401096393 9789027725462 |
| issn | 0067-0057 |
| language | English |
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| series2 | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |
| spelling | Aller, Lawrence Hugh 1913-2003 Verfasser (DE-588)102765529 aut Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae by Lawrence H. Aller Dordrecht Springer Netherlands 1984 1 Online-Ressource (350p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 112 0067-0057 Gaseous nebulae offer outstanding opportunities to atomic physicists, spectroscopists, plasma experts, and to observers and theoreticians alike for the study of attenuated ionized gases. These nebulae are often dusty, heated by radiation fields and by shocks. They are short-lived phenomena on the scale of a stellar lifetime, but their chemical compositions and internal kinematics may give important clues to advanced stages of stellar evolution. The material herein presented is based on lectures given at the University of Michigan, University of Queensland, University of California, Los Angeles, and in more abbreviated form at the Raman Institute, at the Scuola Internazionale di Trieste, and elsewhere. Much of it is derived origionally from the series "Physical Processes in Gaseous Nebulae" initiated at the Harvard College Observatory in the late 1930s. I have tried to emphasize the basic physics of the mechanisms involved and mention some of the uncertainties that underlie calculations of many basic parameters. Emphasis is placed on ionized plasmas with electron temperatures typically in the neighborhood of 10,OOOoK. Dust and other ingredients of the cold component of the interstellar medium are treated briefly from the point of view of their relation to hot plasmas of H II regions and planetaries. Chemical composition determinations for nebulae are discussed in some detail while the last section deals with interpretations of elemental abundances in the framework of stellar evolution and nucleogenesis. Gaseous nebulae offer some particularly engaging opportunities for studies of stellar evolution Physics Astronomy, Observations and Techniques Emissionsnebel (DE-588)4466661-5 gnd rswk-swf Emissionsnebel (DE-588)4466661-5 s 1\p DE-604 https://doi.org/10.1007/978-94-010-9639-3 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Aller, Lawrence Hugh 1913-2003 Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae Physics Astronomy, Observations and Techniques Emissionsnebel (DE-588)4466661-5 gnd |
| subject_GND | (DE-588)4466661-5 |
| title | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae |
| title_auth | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae |
| title_exact_search | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae |
| title_full | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae by Lawrence H. Aller |
| title_fullStr | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae by Lawrence H. Aller |
| title_full_unstemmed | Physics of Thermal Gaseous Nebulae Physical Processes in Gaseous Nebulae by Lawrence H. Aller |
| title_short | Physics of Thermal Gaseous Nebulae |
| title_sort | physics of thermal gaseous nebulae physical processes in gaseous nebulae |
| title_sub | Physical Processes in Gaseous Nebulae |
| topic | Physics Astronomy, Observations and Techniques Emissionsnebel (DE-588)4466661-5 gnd |
| topic_facet | Physics Astronomy, Observations and Techniques Emissionsnebel |
| url | https://doi.org/10.1007/978-94-010-9639-3 |
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