Li abundances in solar-analog stars. II. (Takeda+, 2010)

Details Li abundances in solar-analog stars. II. (Takeda+, 2010) Li abundances in solar-analog stars. II. (Takeda+, 2010)

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35159093t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/515/A93. Originally published in: 2010A&A...515A..93T

Astronomy and Astrophysics

Astrophysics

Stars: Late-Type, Stars: G-Type, Stars: Nearby, Abundances, Effective Temperatures

Scientific paper

To acquire data for studying stellar activities from Ca II near-IR triplet, the observations of 118 solar-analog stars (the same sample as in Paper I, Cat. J/A+A/468/663) were carried out in five different months (2007 February and April; 2008 May, August, and December) by using the HIgh-Dispersion Echelle Spectrograph (HIDES; Izumiura 1999) at the coude focus of the 188cm reflector of Okayama Astrophysical Observatory (OAO).
(1 data file).

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