Pulsation and Mass Loss in Stars: Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1988
|
| 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
148 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales. The study of stellar winds and the effects of stellar mass loss has reached a particularly exciting stage where observational capabilities are increasingly able to provide interesting constraints on models and theories. Recent resu1ts from theoretical and observational work for both hot and cool stars with substantial winds have led to the suggestion that a combination of pulsation with other mechanisms makes for particularly efficient mass loss from stars. This provided the original motivation for the organization of this workshop. The conference was organized along relatively conventional lines according to the types of objects being scrutinized. However the true unity of the proceedings comes from the interplay of the mechanisms involved. For example, for the cool, luminous Mira variables, pulsation leads to shock waves that extend the atmosphere, enhancing dust formation; radiation pressure on dust drives the wind, cooling the atmosphere and in some cases suppressing the shocks. Similarly for the Be stars, both pulsation (in this case, non-radial) and radiation pressure (due to UV resonance lines) are expected to be important, and this expectation is at least qualitatively borne out by the observations |
| Beschreibung: | 1 Online-Ressource (XII, 336 p) |
| ISBN: | 9789400930292 9789401078610 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-009-3029-2 |
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| 500 | |a Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales. The study of stellar winds and the effects of stellar mass loss has reached a particularly exciting stage where observational capabilities are increasingly able to provide interesting constraints on models and theories. Recent resu1ts from theoretical and observational work for both hot and cool stars with substantial winds have led to the suggestion that a combination of pulsation with other mechanisms makes for particularly efficient mass loss from stars. This provided the original motivation for the organization of this workshop. The conference was organized along relatively conventional lines according to the types of objects being scrutinized. However the true unity of the proceedings comes from the interplay of the mechanisms involved. For example, for the cool, luminous Mira variables, pulsation leads to shock waves that extend the atmosphere, enhancing dust formation; radiation pressure on dust drives the wind, cooling the atmosphere and in some cases suppressing the shocks. Similarly for the Be stars, both pulsation (in this case, non-radial) and radiation pressure (due to UV resonance lines) are expected to be important, and this expectation is at least qualitatively borne out by the observations | ||
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Datensatz im Suchindex
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| discipline | Physik |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:56Z |
| institution | BVB |
| isbn | 9789400930292 9789401078610 |
| issn | 0067-0057 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850564 |
| oclc_num | 863762780 |
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| physical | 1 Online-Ressource (XII, 336 p) |
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| publisher | Springer Netherlands |
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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 | Stalio, R. Verfasser aut Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 edited by R. Stalio, L. A. Willson Proceedings of a Workshop held in Trieste, Italy, September 14-18, 1987 Dordrecht Springer Netherlands 1988 1 Online-Ressource (XII, 336 p) 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 148 0067-0057 Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales. The study of stellar winds and the effects of stellar mass loss has reached a particularly exciting stage where observational capabilities are increasingly able to provide interesting constraints on models and theories. Recent resu1ts from theoretical and observational work for both hot and cool stars with substantial winds have led to the suggestion that a combination of pulsation with other mechanisms makes for particularly efficient mass loss from stars. This provided the original motivation for the organization of this workshop. The conference was organized along relatively conventional lines according to the types of objects being scrutinized. However the true unity of the proceedings comes from the interplay of the mechanisms involved. For example, for the cool, luminous Mira variables, pulsation leads to shock waves that extend the atmosphere, enhancing dust formation; radiation pressure on dust drives the wind, cooling the atmosphere and in some cases suppressing the shocks. Similarly for the Be stars, both pulsation (in this case, non-radial) and radiation pressure (due to UV resonance lines) are expected to be important, and this expectation is at least qualitatively borne out by the observations Physics Astronomy, Observations and Techniques Willson, L. A. Sonstige oth https://doi.org/10.1007/978-94-009-3029-2 Verlag Volltext |
| spellingShingle | Stalio, R. Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 Physics Astronomy, Observations and Techniques |
| title | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 |
| title_alt | Proceedings of a Workshop held in Trieste, Italy, September 14-18, 1987 |
| title_auth | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 |
| title_exact_search | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 |
| title_full | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 edited by R. Stalio, L. A. Willson |
| title_fullStr | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 edited by R. Stalio, L. A. Willson |
| title_full_unstemmed | Pulsation and Mass Loss in Stars Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 edited by R. Stalio, L. A. Willson |
| title_short | Pulsation and Mass Loss in Stars |
| title_sort | pulsation and mass loss in stars proceedings of a workshop held in trieste italy september 14 18 1987 |
| title_sub | Proceedings of a Workshop Held in Trieste, Italy, September 14–18, 1987 |
| topic | Physics Astronomy, Observations and Techniques |
| topic_facet | Physics Astronomy, Observations and Techniques |
| url | https://doi.org/10.1007/978-94-009-3029-2 |
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