ABUNDANCES IN G DWARF STARS. III. STARS IN MOVING CLUSTERS
Journal Article
·
· Astrophysical Journal (U.S.)
Abundance determinations were made for three G dwarf stars (one young, two old) that are members of some of Eggen's moving clusters. The metal abundance is roughly solar, but all three stars show a slight overabundance of barium and an underabundance of manganese. One star, HD 30455, appears to have a slight undersbundance of those elements produced by the e-process, compared to those produced by the s-process. (auth) .
- Research Organization:
- Univ. of Rochester, N.Y.
- NSA Number:
- NSA-15-014926
- OSTI ID:
- 4057152
- Report Number(s):
- AFOSR-TN-60-763; 0004-637X
- Journal Information:
- Astrophysical Journal (U.S.), Journal Name: Astrophysical Journal (U.S.) Vol. Vol: 132; ISSN ASJOA
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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