CaltechAUTHORS
  A Caltech Library Service

The Carbon Abundance of Population II Stars

Cohen, J. G. (1968) The Carbon Abundance of Population II Stars. Astrophysical Letters, 2 . pp. 163-164. ISSN 0004-6388. https://resolver.caltech.edu/CaltechAUTHORS:20190610-100620711

[img] PDF - Published Version
See Usage Policy.

180kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190610-100620711

Abstract

Curve of growth analyses available to date for Population II stars have indicated that carbon is more deficient relative to the sun than iron. A refined treatment, which takes into account stratification and molecular equilibrium, shows that carbon is not more deficient than iron, assuming a solar oxygen-to-iron ratio.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1968ApL.....2..163CADSArticle
ORCID:
AuthorORCID
Cohen, J. G.0000-0002-8039-4673
Additional Information:© 1968 Taylor & Francis. Provided by the NASA Astrophysics Data System. Received 28 August 1968. This research has been supported by Grant GP 7030 of the National Science Foundation. The author thanks Professor J. L. Greenstein for suggesting the problem and for helpful discussions, and Dr. S. E. Strom and Mr. R. L. Kurucz for the use of their computer programs.
Funders:
Funding AgencyGrant Number
NSFGP 7030
Record Number:CaltechAUTHORS:20190610-100620711
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190610-100620711
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96235
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Jun 2019 17:14
Last Modified:03 Oct 2019 21:20

Repository Staff Only: item control page