Elemental abundances of the mercury-manganese stars HR 4817 and Chi LUPI

Details Elemental abundances of the mercury-manganese stars HR 4817 and Chi LUPI Elemental abundances of the mercury-manganese stars HR 4817 and Chi LUPI

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...238..111a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 238, no. 1-2, Nov. 1990, p. 111-115.

Astronomy and Astrophysics

Astrophysics

9

Abundance, Manganese, Mercury (Metal), Metallic Stars, Stellar Composition, Charge Coupled Devices, Metallicity, Stellar Spectra

Scientific paper

Fine analyses of limited spectral regions of the mercury-manganese stars
HR 4817 and Chi Lup confirm that these stars have abundances of typical
class members. The best determined values of HR 4817 are similar to
those of 53 Tau which is an anomalous class member.

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