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...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge, UK ; New York :
Cambridge University Press,
2006.
|
| Schriftenreihe: | Cambridge astrophysics series ;
40. |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Zusammenfassung: | 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. |
| Beschreibung: | 1 online resource (viii, 322 pages) : illustrations |
| Bibliographie: | Includes bibliographical references (pages 304-314) and indexes. |
| ISBN: | 9780511226298 0511226292 0511223080 9780511223082 9780511536205 0511536208 9786610550531 6610550530 1107166101 9781107166103 1280550538 9781280550539 0511225725 9780511225727 0511317832 9780511317835 0511225091 9780511225093 |
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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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| _version_ | 1816881651976765440 |
| adam_text | |
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| author | Eggleton, P. P. (Peter P.), 1940- |
| author_GND | http://id.loc.gov/authorities/names/n84200909 |
| author_facet | Eggleton, P. P. (Peter P.), 1940- |
| author_role | |
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| collection | ZDB-4-EBA |
| contents | Cover; Half-title; Series-title; Title; Copyright; Contents; Preface; 1 Introduction; 2 Evolution of single stars; 3 Binary interaction: conservative processes; 4 Slow non-conservative processes; 5 Rapid non-conservative processes; 6 Accretion by the companion; Appendix A The equations of stellar structure; Appendix B Distortion and circulation in a non-spherical star; Appendix C Perturbations to Keplerian orbits; Appendix D Steady, axisymmetric magnetic winds; Appendix E Stellar dynamos; Appendix F Steady, axisymmetric, cool accretion discs; References; Subject index; Stellar objects index |
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| indexdate | 2024-11-27T13:16:07Z |
| institution | BVB |
| isbn | 9780511226298 0511226292 0511223080 9780511223082 9780511536205 0511536208 9786610550531 6610550530 1107166101 9781107166103 1280550538 9781280550539 0511225725 9780511225727 0511317832 9780511317835 0511225091 9780511225093 |
| language | English |
| oclc_num | 163091618 |
| open_access_boolean | |
| owner | MAIN DE-863 DE-BY-FWS |
| owner_facet | MAIN DE-863 DE-BY-FWS |
| physical | 1 online resource (viii, 322 pages) : illustrations |
| psigel | ZDB-4-EBA |
| publishDate | 2006 |
| publishDateSearch | 2006 |
| publishDateSort | 2006 |
| publisher | Cambridge University Press, |
| record_format | marc |
| series | Cambridge astrophysics series ; |
| series2 | Cambridge astrophysics series ; |
| spelling | Eggleton, P. P. (Peter P.), 1940- https://id.oclc.org/worldcat/entity/E39PBJjd9bvcxYFdXvQK6qk4bd http://id.loc.gov/authorities/names/n84200909 Evolutionary processes in binary and multiple stars / Peter Eggleton. Cambridge, UK ; New York : Cambridge University Press, 2006. 1 online resource (viii, 322 pages) : illustrations text txt rdacontent computer c rdamedia online resource cr rdacarrier Cambridge astrophysics series ; 40 Includes bibliographical references (pages 304-314) and indexes. Print version record. 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. Cover; Half-title; Series-title; Title; Copyright; Contents; Preface; 1 Introduction; 2 Evolution of single stars; 3 Binary interaction: conservative processes; 4 Slow non-conservative processes; 5 Rapid non-conservative processes; 6 Accretion by the companion; Appendix A The equations of stellar structure; Appendix B Distortion and circulation in a non-spherical star; Appendix C Perturbations to Keplerian orbits; Appendix D Steady, axisymmetric magnetic winds; Appendix E Stellar dynamos; Appendix F Steady, axisymmetric, cool accretion discs; References; Subject index; Stellar objects index English. Double stars Evolution. http://id.loc.gov/authorities/subjects/sh92002195 Multiple stars. http://id.loc.gov/authorities/subjects/sh85088378 Étoiles doubles Évolution. Étoiles multiples. SCIENCE Astronomy. bisacsh Double stars Evolution fast Multiple stars fast Doppelstern gnd http://d-nb.info/gnd/4150454-9 Mehrfachstern gnd http://d-nb.info/gnd/4334294-2 Sternentwicklung gnd http://d-nb.info/gnd/4057365-5 Print version: Eggleton, P.P. (Peter P.), 1940- Evolutionary processes in binary and multiple stars. Cambridge, UK ; New York : Cambridge University Press, 2006 0521855578 9780521855570 (DLC) 2006299123 (OCoLC)61757144 Cambridge astrophysics series ; 40. http://id.loc.gov/authorities/names/n42034737 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=165327 Volltext |
| spellingShingle | Eggleton, P. P. (Peter P.), 1940- Evolutionary processes in binary and multiple stars / Cambridge astrophysics series ; Cover; Half-title; Series-title; Title; Copyright; Contents; Preface; 1 Introduction; 2 Evolution of single stars; 3 Binary interaction: conservative processes; 4 Slow non-conservative processes; 5 Rapid non-conservative processes; 6 Accretion by the companion; Appendix A The equations of stellar structure; Appendix B Distortion and circulation in a non-spherical star; Appendix C Perturbations to Keplerian orbits; Appendix D Steady, axisymmetric magnetic winds; Appendix E Stellar dynamos; Appendix F Steady, axisymmetric, cool accretion discs; References; Subject index; Stellar objects index Double stars Evolution. http://id.loc.gov/authorities/subjects/sh92002195 Multiple stars. http://id.loc.gov/authorities/subjects/sh85088378 Étoiles doubles Évolution. Étoiles multiples. SCIENCE Astronomy. bisacsh Double stars Evolution fast Multiple stars fast Doppelstern gnd http://d-nb.info/gnd/4150454-9 Mehrfachstern gnd http://d-nb.info/gnd/4334294-2 Sternentwicklung gnd http://d-nb.info/gnd/4057365-5 |
| subject_GND | http://id.loc.gov/authorities/subjects/sh92002195 http://id.loc.gov/authorities/subjects/sh85088378 http://d-nb.info/gnd/4150454-9 http://d-nb.info/gnd/4334294-2 http://d-nb.info/gnd/4057365-5 |
| title | Evolutionary processes in binary and 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. http://id.loc.gov/authorities/subjects/sh92002195 Multiple stars. http://id.loc.gov/authorities/subjects/sh85088378 Étoiles doubles Évolution. Étoiles multiples. SCIENCE Astronomy. bisacsh Double stars Evolution fast Multiple stars fast Doppelstern gnd http://d-nb.info/gnd/4150454-9 Mehrfachstern gnd http://d-nb.info/gnd/4334294-2 Sternentwicklung gnd http://d-nb.info/gnd/4057365-5 |
| topic_facet | Double stars Evolution. Multiple stars. Étoiles doubles Évolution. Étoiles multiples. SCIENCE Astronomy. Double stars Evolution Multiple stars Doppelstern Mehrfachstern Sternentwicklung |
| url | https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=165327 |
| work_keys_str_mv | AT eggletonpp evolutionaryprocessesinbinaryandmultiplestars |