Li abundances in solar-analog stars (Takeda+, 2007)

Details Li abundances in solar-analog stars (Takeda+, 2007) Li abundances in solar-analog stars (Takeda+, 2007)

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34680663t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/468/663. Originally published in: 2007A&A...468..663T

Physics

Stars: Late-Type, Stars: Nearby, Abundances, Equivalent Widths

Scientific paper

The atmospheric parameters were spectroscopically determined by using the equivalent widths of FeI and FeII lines, the ages/masses were estimated from stellar evolutionary tracks, and the width of the macrobroadening (rotation plus macroturbulence) function as well as Li abundances (ALi) were established by spectrum-fitting analyses.
(5 data files).

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