Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..129..563p&link_type=abstract
Astronomy and Astrophysics Supplement, v.129, p.563-567
Astronomy and Astrophysics
Astrophysics
7
Stars: Abundances, Stars: Chemically Peculiar, Stars: Individual: Hr 4487, 14 Hya, 3 Cen A
Scientific paper
Using CASLEO echelle spectrograms, elemental abundances are derived for the sharp-lined non-magnetic CP stars HR 4487, 14 Hya, and 3 Cen A. The first two stars are members of the Mercury-Manganese subgroup and have abundances which are similar to other such peculiar stars. The third is a hotter related star. The detection of Mn II lines in its spectrum adds to this relationship. Table 3 is avaible electronically vit the CDS via anonymous ftp 130.79.128.5 or http://cdsweb.u-strasbg.fr/Abstract.html.
Adelman Saul J.
Gulliver Austin F.
Pintado Olga I.
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