The Symbiotic Phenomenon: Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987
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| 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
145 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Symbiotic stars were identified spectroscopically as M giants with a very strong He II 4686 emission line. After five decades of study by many astronomers, the first internatioinal meetings devoted to symbiotics were held at the University of Colorado (Boulder) and at the Haute Provence Observatory during the Summer of 1981. These conferences emphasized exciting new results obtained by modern satellite (EINSTEIN, IUE) and ground-based observatories. Although the vast majority of the participants were already fairly sure that symbiotics are almost certainly interacting binary systems, and not extremely peculiar single stars, it was not clear exactly which types of physical processes were needed to be invoked to explain their observed behaviour. Many were even worried that it might not be possible to clearly define a class of "symbiotic stars" , and thus establish a unique model applicable to any system. Since the publication of the Haute-Provence proceedings, our understanding of the physical processes occuring in symbiotic stars (and in related objects such as cataclysmic variables and compact planetary nebulae) has greatly improved. We now speak confidently of a "symbiotic phenomenon" , in which an evolved red giant and a hot companion object (usually thought to be an accreting main sequence star or a luminous white dwarf star) happily coexist |
| Beschreibung: | 1 Online-Ressource (380p) |
| ISBN: | 9789400929692 9789401078337 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-009-2969-2 |
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| 500 | |a Symbiotic stars were identified spectroscopically as M giants with a very strong He II 4686 emission line. After five decades of study by many astronomers, the first internatioinal meetings devoted to symbiotics were held at the University of Colorado (Boulder) and at the Haute Provence Observatory during the Summer of 1981. These conferences emphasized exciting new results obtained by modern satellite (EINSTEIN, IUE) and ground-based observatories. Although the vast majority of the participants were already fairly sure that symbiotics are almost certainly interacting binary systems, and not extremely peculiar single stars, it was not clear exactly which types of physical processes were needed to be invoked to explain their observed behaviour. Many were even worried that it might not be possible to clearly define a class of "symbiotic stars" , and thus establish a unique model applicable to any system. Since the publication of the Haute-Provence proceedings, our understanding of the physical processes occuring in symbiotic stars (and in related objects such as cataclysmic variables and compact planetary nebulae) has greatly improved. We now speak confidently of a "symbiotic phenomenon" , in which an evolved red giant and a hot companion object (usually thought to be an accreting main sequence star or a luminous white dwarf star) happily coexist | ||
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| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-2969-2 |
| format | Electronic eBook |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:56Z |
| institution | BVB |
| isbn | 9789400929692 9789401078337 |
| 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 | Mikolajewska, Joanna Verfasser aut The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 edited by Joanna Mikolajewska, Michael Friedjung, Scott J. Kenyon, Roberto Viotti Proceedings of the 103rd Colloquium of the International Astronomical Union, held in Torun, Poland, August 18-20, 1987 Dordrecht Springer Netherlands 1988 1 Online-Ressource (380p) 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 145 0067-0057 Symbiotic stars were identified spectroscopically as M giants with a very strong He II 4686 emission line. After five decades of study by many astronomers, the first internatioinal meetings devoted to symbiotics were held at the University of Colorado (Boulder) and at the Haute Provence Observatory during the Summer of 1981. These conferences emphasized exciting new results obtained by modern satellite (EINSTEIN, IUE) and ground-based observatories. Although the vast majority of the participants were already fairly sure that symbiotics are almost certainly interacting binary systems, and not extremely peculiar single stars, it was not clear exactly which types of physical processes were needed to be invoked to explain their observed behaviour. Many were even worried that it might not be possible to clearly define a class of "symbiotic stars" , and thus establish a unique model applicable to any system. Since the publication of the Haute-Provence proceedings, our understanding of the physical processes occuring in symbiotic stars (and in related objects such as cataclysmic variables and compact planetary nebulae) has greatly improved. We now speak confidently of a "symbiotic phenomenon" , in which an evolved red giant and a hot companion object (usually thought to be an accreting main sequence star or a luminous white dwarf star) happily coexist Physics Astrophysics and Astroparticles Friedjung, Michael Sonstige oth Kenyon, Scott J. Sonstige oth Viotti, Roberto Sonstige oth https://doi.org/10.1007/978-94-009-2969-2 Verlag Volltext |
| spellingShingle | Mikolajewska, Joanna The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 Physics Astrophysics and Astroparticles |
| title | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 |
| title_alt | Proceedings of the 103rd Colloquium of the International Astronomical Union, held in Torun, Poland, August 18-20, 1987 |
| title_auth | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 |
| title_exact_search | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 |
| title_full | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 edited by Joanna Mikolajewska, Michael Friedjung, Scott J. Kenyon, Roberto Viotti |
| title_fullStr | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 edited by Joanna Mikolajewska, Michael Friedjung, Scott J. Kenyon, Roberto Viotti |
| title_full_unstemmed | The Symbiotic Phenomenon Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 edited by Joanna Mikolajewska, Michael Friedjung, Scott J. Kenyon, Roberto Viotti |
| title_short | The Symbiotic Phenomenon |
| title_sort | the symbiotic phenomenon proceedings of the 103rd colloquium of the international astronomical union held in torun poland august 18 20 1987 |
| title_sub | Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987 |
| topic | Physics Astrophysics and Astroparticles |
| topic_facet | Physics Astrophysics and Astroparticles |
| url | https://doi.org/10.1007/978-94-009-2969-2 |
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