Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)

Details Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998) Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..41290563p&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/129/563. Originally published in: 1998A&AS..129..563P

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Stars: Peculiar, Abundances: Peculiar

Scientific paper

Ussing 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.
(2 data files).

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