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THERMAL STRUCTURE OF CONVECTING CARBON-OXYGEN CORES
- Date Issued:
- 1975
- Summary:
- The evolution of the carbon-oxygen cores of intermediate mass stars immediately prior to and following carbon ignition is described. The thermal consequences of the convectively driven URCA process are considered in detail and applied to these cores following carbon ignition to determine their thermal. We found, as did Paczynski and Ergma, and Couch and Arnett, that a global thermal balance and stability is possible for some models. Unlike the previous investigators, however, we found that some models were possibly unstable due to local heating at the edge of the convective region. The implications for intermediate mass stars burning carbon are potentially serious, as these stars naturally evolve into the region occupied by these unstable models.
Title: | THERMAL STRUCTURE OF CONVECTING CARBON-OXYGEN CORES. |
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Name(s): |
ROWLAND, WILLIAM COLWELL. Florida Atlantic University, Degree grantor |
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Type of Resource: | text | |
Genre: | Electronic Thesis Or Dissertation | |
Issuance: | monographic | |
Date Issued: | 1975 | |
Publisher: | Florida Atlantic University | |
Place of Publication: | Boca Raton, Fla. | |
Physical Form: | application/pdf | |
Extent: | 72 p. | |
Language(s): | English | |
Summary: | The evolution of the carbon-oxygen cores of intermediate mass stars immediately prior to and following carbon ignition is described. The thermal consequences of the convectively driven URCA process are considered in detail and applied to these cores following carbon ignition to determine their thermal. We found, as did Paczynski and Ergma, and Couch and Arnett, that a global thermal balance and stability is possible for some models. Unlike the previous investigators, however, we found that some models were possibly unstable due to local heating at the edge of the convective region. The implications for intermediate mass stars burning carbon are potentially serious, as these stars naturally evolve into the region occupied by these unstable models. | |
Identifier: | 13740 (digitool), FADT13740 (IID), fau:10572 (fedora) | |
Collection: | FAU Electronic Theses and Dissertations Collection | |
Note(s): |
Thesis (M.S.)--Florida Atlantic University, 1975. Charles E. Schmidt College of Science |
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Subject(s): |
Thermal analysis Stars--Evolution Supernovae |
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Held by: | Florida Atlantic University Libraries | |
Persistent Link to This Record: | http://purl.flvc.org/fcla/dt/13740 | |
Sublocation: | Digital Library | |
Use and Reproduction: | Copyright © is held by the author with permission granted to Florida Atlantic University to digitize, archive and distribute this item for non-profit research and educational purposes. Any reuse of this item in excess of fair use or other copyright exemptions requires permission of the copyright holder. | |
Use and Reproduction: | http://rightsstatements.org/vocab/InC/1.0/ | |
Host Institution: | FAU | |
Is Part of Series: | Florida Atlantic University Digital Library Collections. |