Active Close Binaries:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1990
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
319 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Since the 1970s symposia or colloquia devoted to recent research on close binaries have been held around the world almost annually. At meetings of the General Assembly of the International Astronomical Union this topic has also been discussed in detail at presentations in various commission meetings and also as invited talks by leading astronomers in the field. In recent years, fundamental changes have taken place in the study of close binaries due to the improvements in observational techniques, extension of observations from X-ray to radio regions of the electromagnetic spectrum, and advances in theoretical studies. For more than a decade, a group of astronomers at Ege University Observatory has been concentrating on active close binaries with particular emphasis on the behaviour of the light curves of chromospherically active systems. Thus, we decided to organize an international meeting in Western Anatolia, where this part of Turkey had been the cradle for great developments in science during antiquity. KUljadasi, located only minutes away from Ephesus, one of the seven wonders of the world, was selected to be the meeting site. Close binary systems constitute a very rich source of information about the physical properties of the component stars. Some systems are eclipsing variables, where periodic recurrences of eclipses are observed as comparatively brief decreases in the total brightness of the binary system. Precise methods of photometric observations make it possible to obtain the light variations of these systems because of eclipses and other phenomena |
| Beschreibung: | 1 Online-Ressource (920p) |
| ISBN: | 9789400906792 9789401067904 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-009-0679-2 |
Internformat
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| 246 | 1 | 3 | |a Proceedings of the NATO Advanced Study Institute, Kusadasi, Turkey, September 11-22, 1989 |
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| 500 | |a Since the 1970s symposia or colloquia devoted to recent research on close binaries have been held around the world almost annually. At meetings of the General Assembly of the International Astronomical Union this topic has also been discussed in detail at presentations in various commission meetings and also as invited talks by leading astronomers in the field. In recent years, fundamental changes have taken place in the study of close binaries due to the improvements in observational techniques, extension of observations from X-ray to radio regions of the electromagnetic spectrum, and advances in theoretical studies. For more than a decade, a group of astronomers at Ege University Observatory has been concentrating on active close binaries with particular emphasis on the behaviour of the light curves of chromospherically active systems. Thus, we decided to organize an international meeting in Western Anatolia, where this part of Turkey had been the cradle for great developments in science during antiquity. KUljadasi, located only minutes away from Ephesus, one of the seven wonders of the world, was selected to be the meeting site. Close binary systems constitute a very rich source of information about the physical properties of the component stars. Some systems are eclipsing variables, where periodic recurrences of eclipses are observed as comparatively brief decreases in the total brightness of the binary system. Precise methods of photometric observations make it possible to obtain the light variations of these systems because of eclipses and other phenomena | ||
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Datensatz im Suchindex
| _version_ | 1804153081315721217 |
|---|---|
| any_adam_object | |
| author | İbanoğlu, Cafer |
| author_facet | İbanoğlu, Cafer |
| author_role | aut |
| author_sort | İbanoğlu, Cafer |
| author_variant | c i ci |
| building | Verbundindex |
| bvnumber | BV042414921 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)906741966 (DE-599)BVBBV042414921 |
| 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 | 10.1007/978-94-009-0679-2 |
| format | Electronic eBook |
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| spelling | İbanoğlu, Cafer Verfasser aut Active Close Binaries edited by Cafer İbanoğlu Proceedings of the NATO Advanced Study Institute, Kusadasi, Turkey, September 11-22, 1989 Dordrecht Springer Netherlands 1990 1 Online-Ressource (920p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 319 1389-2185 Since the 1970s symposia or colloquia devoted to recent research on close binaries have been held around the world almost annually. At meetings of the General Assembly of the International Astronomical Union this topic has also been discussed in detail at presentations in various commission meetings and also as invited talks by leading astronomers in the field. In recent years, fundamental changes have taken place in the study of close binaries due to the improvements in observational techniques, extension of observations from X-ray to radio regions of the electromagnetic spectrum, and advances in theoretical studies. For more than a decade, a group of astronomers at Ege University Observatory has been concentrating on active close binaries with particular emphasis on the behaviour of the light curves of chromospherically active systems. Thus, we decided to organize an international meeting in Western Anatolia, where this part of Turkey had been the cradle for great developments in science during antiquity. KUljadasi, located only minutes away from Ephesus, one of the seven wonders of the world, was selected to be the meeting site. Close binary systems constitute a very rich source of information about the physical properties of the component stars. Some systems are eclipsing variables, where periodic recurrences of eclipses are observed as comparatively brief decreases in the total brightness of the binary system. Precise methods of photometric observations make it possible to obtain the light variations of these systems because of eclipses and other phenomena Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Veränderlicher Stern (DE-588)4062534-5 gnd rswk-swf Doppelstern (DE-588)4150454-9 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1989 Kuşadasi gnd-content Veränderlicher Stern (DE-588)4062534-5 s 2\p DE-604 Doppelstern (DE-588)4150454-9 s 3\p DE-604 https://doi.org/10.1007/978-94-009-0679-2 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 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | İbanoğlu, Cafer Active Close Binaries Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Veränderlicher Stern (DE-588)4062534-5 gnd Doppelstern (DE-588)4150454-9 gnd |
| subject_GND | (DE-588)4062534-5 (DE-588)4150454-9 (DE-588)1071861417 |
| title | Active Close Binaries |
| title_alt | Proceedings of the NATO Advanced Study Institute, Kusadasi, Turkey, September 11-22, 1989 |
| title_auth | Active Close Binaries |
| title_exact_search | Active Close Binaries |
| title_full | Active Close Binaries edited by Cafer İbanoğlu |
| title_fullStr | Active Close Binaries edited by Cafer İbanoğlu |
| title_full_unstemmed | Active Close Binaries edited by Cafer İbanoğlu |
| title_short | Active Close Binaries |
| title_sort | active close binaries |
| topic | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Veränderlicher Stern (DE-588)4062534-5 gnd Doppelstern (DE-588)4150454-9 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Veränderlicher Stern Doppelstern Konferenzschrift 1989 Kuşadasi |
| url | https://doi.org/10.1007/978-94-009-0679-2 |
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