Catalog Service: Abundances of HR 4487, 14 Hyd and 3 Cen A
Description
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.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2000 Jan 19 20:59:13ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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