The Atmospheric Lithium Abundances of Solar Analogues

Details The Atmospheric Lithium Abundances of Solar Analogues The Atmospheric Lithium Abundances of Solar Analogues

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004arep...48..511g&link_type=abstract

Astronomy Reports, Volume 48, Issue 6, p.511-521

Astronomy and Astrophysics

Astronomy

3

Scientific paper

We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based on high-resolution echelle spectra using model atmospheres in a non-LTE approach. In terms of their lithium abundances, the stars (which are located in a narrow range of temperatures of 5650 5900 K) can be divided into two groups: one with low lithium abundances, as in the solar atmosphere, and one with lithium abundances that are higher than the solar value by about 1 dex (with the accuracy of the lithium abundances being 0.15 dex).

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