On the cobalt abundances of early-type stars

Details On the cobalt abundances of early-type stars On the cobalt abundances of early-type stars

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...353..335a&link_type=abstract

Astronomy and Astrophysics, v.353, p.335-338 (2000)

Astronomy and Astrophysics

Astrophysics

5

Stars: Abundances, Stars: Chemically Peculiar

Scientific paper

Photographic region high-dispersion high signal-to-noise spectra of A and F main sequence band stars which exhibit modest rotation show Co I lines. In the hottest of these stars, we also found weak Co II lines whose abundances are consistent with those from Co I lines. As a class the Am stars have cobalt abundances which are greater than solar while the normal stars have solar values.

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