The Main Sequence Width - Effects of Age Metallicity and Helium Abundance

Details The Main Sequence Width - Effects of Age Metallicity and Helium Abundance The Main Sequence Width - Effects of Age Metallicity and Helium Abundance

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1514....1s&link_type=abstract

Astronomicheskii Tsirkulyar NO.1514/OCT, P. 1, 1987

Astronomy and Astrophysics

Astronomy

Scientific paper

It is shown that the main sequence width for F stars of a given
metallicity can hardly be explained by age spread only and requires
probably a significant helium abundance spread as well.

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