Evolution of Massive Stars: A Confrontation between Theory and Observation
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1994
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| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Massive stars occupy an exceptional place in general astrophysics. They trigger many if not all of the important processes in galactic evolution whereas due to their intrinsic brightness, they offer the (only until now) possibility to study the stellar content and stellar behaviour in distant galaxies. The last, say, 25 years, massive stars have been the subject of numerous meetings discussing the influence of massive stars on population synthesis, the number distribution of different types of massive stars, the LBV phenomenon, WR stars, X-ray binaries, stellar winds in massive stars, chemical pecularities in massive stars, supernova explosions of massive stars and the important SN1987A event, the influence of massive stars and chemical evolution of galaxies. It is clear that without a theory of stellar evolution, the study of these topics loses a lot of its significance. Massive star evolution therefore got a chance in these meetings, but rarely as a prime subject. The state of the art, the physical processes and the uncertainties in stellar evolution were barely touched. Even more, the influence of close binaries in all these massive star meetings slowly disappeared the last, say, 13 years without any scientific justification, although a significant fraction of stars occurs in close binaries with periods small enough so that both components will interact during their evolution. Denying the binaries or not discussing their influence on results and conclusions, makes the latter very uncertain or even completely unreliable |
| Beschreibung: | 1 Online-Ressource (VII, 490 p) |
| ISBN: | 9789401110808 9789401044714 |
| DOI: | 10.1007/978-94-011-1080-8 |
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| 500 | |a Massive stars occupy an exceptional place in general astrophysics. They trigger many if not all of the important processes in galactic evolution whereas due to their intrinsic brightness, they offer the (only until now) possibility to study the stellar content and stellar behaviour in distant galaxies. The last, say, 25 years, massive stars have been the subject of numerous meetings discussing the influence of massive stars on population synthesis, the number distribution of different types of massive stars, the LBV phenomenon, WR stars, X-ray binaries, stellar winds in massive stars, chemical pecularities in massive stars, supernova explosions of massive stars and the important SN1987A event, the influence of massive stars and chemical evolution of galaxies. It is clear that without a theory of stellar evolution, the study of these topics loses a lot of its significance. Massive star evolution therefore got a chance in these meetings, but rarely as a prime subject. The state of the art, the physical processes and the uncertainties in stellar evolution were barely touched. Even more, the influence of close binaries in all these massive star meetings slowly disappeared the last, say, 13 years without any scientific justification, although a significant fraction of stars occurs in close binaries with periods small enough so that both components will interact during their evolution. Denying the binaries or not discussing their influence on results and conclusions, makes the latter very uncertain or even completely unreliable | ||
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| dewey-hundreds | 500 - Natural sciences and mathematics |
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| discipline | Physik |
| doi_str_mv | 10.1007/978-94-011-1080-8 |
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| spelling | Vanbeveren, D. Verfasser aut Evolution of Massive Stars A Confrontation between Theory and Observation edited by D. Vanbeveren, W. Rensbergen, C. Loore Dordrecht Springer Netherlands 1994 1 Online-Ressource (VII, 490 p) txt rdacontent c rdamedia cr rdacarrier Massive stars occupy an exceptional place in general astrophysics. They trigger many if not all of the important processes in galactic evolution whereas due to their intrinsic brightness, they offer the (only until now) possibility to study the stellar content and stellar behaviour in distant galaxies. The last, say, 25 years, massive stars have been the subject of numerous meetings discussing the influence of massive stars on population synthesis, the number distribution of different types of massive stars, the LBV phenomenon, WR stars, X-ray binaries, stellar winds in massive stars, chemical pecularities in massive stars, supernova explosions of massive stars and the important SN1987A event, the influence of massive stars and chemical evolution of galaxies. It is clear that without a theory of stellar evolution, the study of these topics loses a lot of its significance. Massive star evolution therefore got a chance in these meetings, but rarely as a prime subject. The state of the art, the physical processes and the uncertainties in stellar evolution were barely touched. Even more, the influence of close binaries in all these massive star meetings slowly disappeared the last, say, 13 years without any scientific justification, although a significant fraction of stars occurs in close binaries with periods small enough so that both components will interact during their evolution. Denying the binaries or not discussing their influence on results and conclusions, makes the latter very uncertain or even completely unreliable Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles Sternentwicklung (DE-588)4057365-5 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1993 Brüssel gnd-content Sternentwicklung (DE-588)4057365-5 s 2\p DE-604 Rensbergen, W. Sonstige oth Loore, C. Sonstige oth https://doi.org/10.1007/978-94-011-1080-8 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Vanbeveren, D. Evolution of Massive Stars A Confrontation between Theory and Observation Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles Sternentwicklung (DE-588)4057365-5 gnd |
| subject_GND | (DE-588)4057365-5 (DE-588)1071861417 |
| title | Evolution of Massive Stars A Confrontation between Theory and Observation |
| title_auth | Evolution of Massive Stars A Confrontation between Theory and Observation |
| title_exact_search | Evolution of Massive Stars A Confrontation between Theory and Observation |
| title_full | Evolution of Massive Stars A Confrontation between Theory and Observation edited by D. Vanbeveren, W. Rensbergen, C. Loore |
| title_fullStr | Evolution of Massive Stars A Confrontation between Theory and Observation edited by D. Vanbeveren, W. Rensbergen, C. Loore |
| title_full_unstemmed | Evolution of Massive Stars A Confrontation between Theory and Observation edited by D. Vanbeveren, W. Rensbergen, C. Loore |
| title_short | Evolution of Massive Stars |
| title_sort | evolution of massive stars a confrontation between theory and observation |
| title_sub | A Confrontation between Theory and Observation |
| topic | Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles Sternentwicklung (DE-588)4057365-5 gnd |
| topic_facet | Physics Astronomy, Observations and Techniques Astrophysics and Astroparticles Sternentwicklung Konferenzschrift 1993 Brüssel |
| url | https://doi.org/10.1007/978-94-011-1080-8 |
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