Lithium Abundances in Orion IC PMS Stars

Details Lithium Abundances in Orion IC PMS Stars Lithium Abundances in Orion IC PMS Stars

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.2609k&link_type=abstract

American Astronomical Society, 180th AAS Meeting, #26.09; Bulletin of the American Astronomical Society, Vol. 24, p.768

Astronomy and Astrophysics

Astronomy

Scientific paper

I present (7) Li abundances for 23 intermediate-mass (1.5=}5500 K) temperatures. Such a spread can not be explained by either standard models or the new rotational Yale models. Because the stars with the smallest rotational velocities also have the lowest Li abundances, I speculate that the explanation for this spread is that rotational braking, leading to mixing and subsequent (7) Li depletion, has occurred within 10(7) yr for some of the stars.

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