Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1422
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Koch, R. H | - |
dc.date.accessioned | 2007-03-14T08:13:37Z | - |
dc.date.available | 2007-03-14T08:13:37Z | - |
dc.date.issued | 1990 | - |
dc.identifier.citation | BASI, Vol. 18, pp. 277-284 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1422 | - |
dc.description.abstract | A review is made of the chemical abundances of binary stars in the catalogs of Cayrel de Strobel (1981, 1985). Solar-type single-line close binaries, A- and B-type close binaries on and near the main sequence, and close binaries with spotted photospheres are considered. It is shown that ignorance of the binary condition introduces a bias into elemental abundance statistics which is of the order of the precision with which an abundance can be ordinarily established. It is also shown that specific-seeming abundance anomalies for hot and cool binaries might be explained by the existence of unrecognized binaries among the sample | en |
dc.format.extent | 286555 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.subject | Close Binaries | en |
dc.subject | Chemical abundances | en |
dc.title | On the chemical abundances of close binary stars on and near the main sequence | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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paper-16.pdf | 279.84 kB | Adobe PDF | ![]() View/Open |
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