Double Stars:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1978
|
| Schriftenreihe: | Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks
15 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: The patterns of evolution involving mass transfer appear to lead ultimately to single objects |
| Beschreibung: | 1 Online-Ressource (X, 175 p) |
| ISBN: | 9789400998360 9789027708861 |
| DOI: | 10.1007/978-94-009-9836-0 |
Internformat
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| 500 | |a Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: The patterns of evolution involving mass transfer appear to lead ultimately to single objects | ||
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Datensatz im Suchindex
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|---|---|
| any_adam_object | |
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| author_facet | Heintz, Wulff D. |
| author_role | aut |
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| author_variant | w d h wd wdh |
| building | Verbundindex |
| bvnumber | BV042415469 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)905420482 (DE-599)BVBBV042415469 |
| 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 | 10.1007/978-94-009-9836-0 |
| format | Electronic eBook |
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| id | DE-604.BV042415469 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789400998360 9789027708861 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850962 |
| oclc_num | 905420482 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (X, 175 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1978 |
| publishDateSearch | 1978 |
| publishDateSort | 1978 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks |
| spelling | Heintz, Wulff D. Verfasser aut Double Stars by Wulff D. Heintz Dordrecht Springer Netherlands 1978 1 Online-Ressource (X, 175 p) txt rdacontent c rdamedia cr rdacarrier Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks 15 Double and multiple stars are the rule in the stellar population, and single stars the minority, as the abundance of binary systems in the space surrounding the sun shows beyond doubt. Numerous stellar features, and methods of their exploration, ensue specifically from the one but widespread property, the binary nature. Stellar masses are basic quantities for the theory of stellar structure and evolution, and they are ob tained from binary-star orbits where they depend on the cube of observed parameters; this fact illustrates the significance of orbits as well as the accuracy requirements. Useful in dating stellar history is the knowledge that components of a system, different though they may appear, are of the same origin and age. Between star formation and the genesis of binaries a direct connection can be traced. The later stages of stellar life branch into a great variety as mutual influence between the components of a close binary pair develops. Transfer and exchange of mass and the presence of angular momentum in the orbit give rise to special tracks of evolution, not found for single stars, and to peculiar spectral groups. This is not a new story but it has a new ending: The patterns of evolution involving mass transfer appear to lead ultimately to single objects Physics Astrophysics and Astroparticles Doppelstern (DE-588)4150454-9 gnd rswk-swf Doppelstern (DE-588)4150454-9 s 1\p DE-604 https://doi.org/10.1007/978-94-009-9836-0 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Heintz, Wulff D. Double Stars Physics Astrophysics and Astroparticles Doppelstern (DE-588)4150454-9 gnd |
| subject_GND | (DE-588)4150454-9 |
| title | Double Stars |
| title_auth | Double Stars |
| title_exact_search | Double Stars |
| title_full | Double Stars by Wulff D. Heintz |
| title_fullStr | Double Stars by Wulff D. Heintz |
| title_full_unstemmed | Double Stars by Wulff D. Heintz |
| title_short | Double Stars |
| title_sort | double stars |
| topic | Physics Astrophysics and Astroparticles Doppelstern (DE-588)4150454-9 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Doppelstern |
| url | https://doi.org/10.1007/978-94-009-9836-0 |
| work_keys_str_mv | AT heintzwulffd doublestars |