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Analysis of F and G Subdwarfs. III. An Abundance Analysis of the Subdwarf μ Cassiopeia

Cohen, Judith G. (1968) Analysis of F and G Subdwarfs. III. An Abundance Analysis of the Subdwarf μ Cassiopeia. Astrophysical Journal, 154 . pp. 179-184. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190529-103831756

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Abstract

Equivalent widths of lines with λ > 4600 Å were measured from a set of 4.5 Å mm^(-1) Palomar plates and were used in performing a model-atmosphere abundance analysis of the mild subdwarf µ Cas. Comparison with the Sun was made by computing abundances from individual solar lines using the same set of transition probabilities as was used for the subdwarf. Results of this analysis show that the iron-peak elements appear to be deficient by a factor of 4, while the α process in µ Cas elements may be enhanced with respect to these elements.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/149748DOIArticle
http://adsabs.harvard.edu/abs/1968ApJ...154..179CADSArticle
ORCID:
AuthorORCID
Cohen, Judith G.0000-0002-8039-4673
Additional Information:© American Astronomical Society • Provided by the NASA Astrophysics Data System. Received August 23,1967; revised April 8, 1968. I would like to thank Dr. J. B. Oke for the use of his plates, Dr. W. Parkinson of Harvard College Observatory for permission to use the David Mann microphotometer, Dr. Stephen Strom and Mr. R. Kurucz for the use of their programs and for helpful discussion. This research has been supported in part by grant NGR 22-024 001 from the National Aeronautics and Space Administration.
Funders:
Funding AgencyGrant Number
NASANGR 22-024 001
Record Number:CaltechAUTHORS:20190529-103831756
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190529-103831756
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95851
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:29 May 2019 21:59
Last Modified:03 Oct 2019 21:17

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