Published January 1968
| Published
Journal Article
Open
Limits on the C^(12)/C^(13)Ratio in Metal-Deficient Stars
- Creators
-
Cohen, J. G.
- Grasdalen, G. L.
Abstract
Lower limits for the ratio C^(12)/C^(13) have been determined for eight metal-deficient stars. These limits are inconsistent with the predictions of nearly all of the universal models considered by Wagoner, Fowler, and Hoyle (1967) unless at least one generation of massive, rapidly evolving stars existed before the formation of any of the program stars.
Additional Information
© American Astronomical Society • Provided by the NASA Astrophysics Data System. Received October 25, 1967. This research has been supported in part by grant NGR 22-024-001 from the National Aeronautics and Space Administration and grant GP 7030 of the National Science Foundation. We should like to thank Prof. W. A. Fowler and Dr. R. Wagoner for helpful discussions. We thank Prof. Jesse L. Greenstein for the plate material. We are very grateful to Dr. Stephen E. Strom, who suggested the problem and provided funds and encouragement.Attached Files
Published - 1968ApJ___151L__41C.pdf
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1968ApJ___151L__41C.pdf
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Additional details
- Eprint ID
- 95849
- Resolver ID
- CaltechAUTHORS:20190529-103831576
- NGR 22-024-001
- NASA
- GP 7030
- NSF
- Created
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2019-05-29Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field