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Elemental abundances of the B6 IV star Xi OctantisAn elemental abundance study used AAT echelle spectrograms of the ultrasharp-lined, superficially normal B6 IV star Xi Octantis. The derived abundances fall within the trends of values derived for normal B main-sequence band stars. On average, they are 0.28 dex less than solar.
Document ID
19930054657
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/133158
Authors
Adelman, Saul J. (The Citadel Charleston, SC, United States)
Robinson, Richard D. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Wahlgren, Glenn M. (Computer Sciences Corp.; NASA, Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
April 1, 1993
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 105
Issue: 686
ISSN: 0004-6280
Subject Category
Astrophysics
Accession Number
93A38654
Funding Number(s)
CONTRACT_GRANT: NAG5-1551
CONTRACT_GRANT: NAG5-921
Distribution Limits
Public
Copyright
Other

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