The metal-to-hydrogen ratio in F1 - F5 stars, as determined by a model-atmosphere analysis of photoelectric observations of a group of weak metal lines.

Details The metal-to-hydrogen ratio in F1 - F5 stars, as determined by a model-atmosphere analysis of photoelectric observations of a group of weak metal lines. The metal-to-hydrogen ratio in F1 - F5 stars, as determined by a model-atmosphere analysis of photoelectric observations of a group of weak metal lines.

Jul 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972a%26a....19..261g&link_type=gif

Astronomy and Astrophysics, Vol. 19, p. 261 - 282

Astronomy and Astrophysics

Astrophysics

68

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1972A&A....19..261G

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