Evolutionary processes in binary and multiple stars:
Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become u...
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2006
|
| Series: | Cambridge astrophysics
40 |
| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (viii, 322 pages) |
| ISBN: | 9780511536205 |
| DOI: | 10.1017/CBO9780511536205 |
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| 520 | |a Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes | ||
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| isbn | 9780511536205 |
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| spelling | Eggleton, P. P. 1940- Verfasser aut Evolutionary processes in binary and multiple stars Peter Eggleton Evolutionary Processes in Binary & Multiple Stars Cambridge Cambridge University Press 2006 1 online resource (viii, 322 pages) txt rdacontent c rdamedia cr rdacarrier Cambridge astrophysics 40 Title from publisher's bibliographic system (viewed on 05 Oct 2015) Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes Double stars / Evolution Multiple stars Mehrfachstern (DE-588)4334294-2 gnd rswk-swf Doppelstern (DE-588)4150454-9 gnd rswk-swf Sternentwicklung (DE-588)4057365-5 gnd rswk-swf Doppelstern (DE-588)4150454-9 s Mehrfachstern (DE-588)4334294-2 s Sternentwicklung (DE-588)4057365-5 s 1\p DE-604 Erscheint auch als Druckausgabe 978-0-521-85557-0 Erscheint auch als Druckausgabe 978-1-107-40342-0 https://doi.org/10.1017/CBO9780511536205 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Eggleton, P. P. 1940- Evolutionary processes in binary and multiple stars Double stars / Evolution Multiple stars Mehrfachstern (DE-588)4334294-2 gnd Doppelstern (DE-588)4150454-9 gnd Sternentwicklung (DE-588)4057365-5 gnd |
| subject_GND | (DE-588)4334294-2 (DE-588)4150454-9 (DE-588)4057365-5 |
| title | Evolutionary processes in binary and multiple stars |
| title_alt | Evolutionary Processes in Binary & Multiple Stars |
| title_auth | Evolutionary processes in binary and multiple stars |
| title_exact_search | Evolutionary processes in binary and multiple stars |
| title_full | Evolutionary processes in binary and multiple stars Peter Eggleton |
| title_fullStr | Evolutionary processes in binary and multiple stars Peter Eggleton |
| title_full_unstemmed | Evolutionary processes in binary and multiple stars Peter Eggleton |
| title_short | Evolutionary processes in binary and multiple stars |
| title_sort | evolutionary processes in binary and multiple stars |
| topic | Double stars / Evolution Multiple stars Mehrfachstern (DE-588)4334294-2 gnd Doppelstern (DE-588)4150454-9 gnd Sternentwicklung (DE-588)4057365-5 gnd |
| topic_facet | Double stars / Evolution Multiple stars Mehrfachstern Doppelstern Sternentwicklung |
| url | https://doi.org/10.1017/CBO9780511536205 |
| work_keys_str_mv | AT eggletonpp evolutionaryprocessesinbinaryandmultiplestars AT eggletonpp evolutionaryprocessesinbinarymultiplestars |