A Grid of Synthetic Spectra for the Determination of Effective Temperature Gravity and Metallicity of F-Stars G-Stars and K-Stars - Part Two - Application to 41 Stellar Spectra Taken in the Basel Field of SA:141

Details A Grid of Synthetic Spectra for the Determination of Effective Temperature Gravity and Metallicity of F-Stars G-Stars and K-Stars - Part Two - Application to 41 Stellar Spectra Taken in the Basel Field of SA:141 A Grid of Synthetic Spectra for the Determination of Effective Temperature Gravity and Metallicity of F-Stars G-Stars and K-Stars - Part Two - Application to 41 Stellar Spectra Taken in the Basel Field of SA:141

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...247..122c&link_type=abstract

Astronomy and Astrophysics, Vol. 247, NO. 1/JULI, P. 122, 1991

Astronomy and Astrophysics

Astrophysics

19

Basel Field Sa 141, Stellar Populations, Synthetic Spectra, Stellar Atmospheric Parameters

Scientific paper

A grid of synthetic spectra is used to derive the atmospheric parameters temperature Teff, gravity log g and metallicity [M/H], besides the radial velocity, from low-resolution spectra of 41 stars in the Basel field SA 141 in the direction of the south galactic pole (l = 245°.0, b = -85°.8).
The metallicity distribution as a function of distance from the galactic plane is obtained and discussed.

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