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Elemental abundances of the mercury-manganese stars HR 4817 and Chi LupiFine 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.
Document ID
19910033540
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Adelman, S. J.
(The Citadel Charleston, SC, United States)
Davis Philip, A. G.
(Union College, Schenectady, NY; Van Vleck Observatory, Middletown CT, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1990
Publication Information
Publication: Astronomy and Astrophysics
Volume: 238
Issue: 2-Jan
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
91A18163
Funding Number(s)
CONTRACT_GRANT: NAG5-921
Distribution Limits
Public
Copyright
Other

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