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An abundance analysis of Tau Herculis, B5 IVAn abundance analysis of the sharp-lined star Tau Herculis (B5 IV) has been performed using a fully line-blanketed model atmosphere. The derived abundances are similar to those of the sun and the normal main-sequence B stars Iota Her (B3 V) and Nu Cap (B9 V).
Document ID
19780033255
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Adelman, S. J.
Date Acquired
August 9, 2013
Publication Date
December 1, 1977
Publication Information
Publication: Royal Astronomical Society
Subject Category
Astrophysics
Accession Number
78A17164
Funding Number(s)
CONTRACT_GRANT: NSG-5055
Distribution Limits
Public
Copyright
Other

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