Lithium Abundances in α Persei Stars

Details Lithium Abundances in α Persei Stars Lithium Abundances in α Persei Stars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005apj...622..620x&link_type=abstract

The Astrophysical Journal, Volume 622, Issue 1, pp. 620-628.

Astronomy and Astrophysics

Astronomy

9

Galaxy: Open Clusters And Associations: Individual: Name: Α Persei, Stars: Abundances, Stars: Activity, Stars: Late-Type

Scientific paper

We revisit the scatter in lithium abundances among stars in the α Persei cluster. Among the factors that we examine, inhomogeneous reddening, stellar spots, and stellar surface activity are the main contributors to this scatter. Thus there is no solid evidence requiring the observed dispersion in lithium abundances to be intrinsic to the cluster member stars. Instead, the scatter is probably induced by observational effects.

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