The Metal Content in the Atmosphere of the Bright Component Upsilon-Sagittarii

Details The Metal Content in the Atmosphere of the Bright Component Upsilon-Sagittarii The Metal Content in the Atmosphere of the Bright Component Upsilon-Sagittarii

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988afz....28..363l&link_type=abstract

Astrofizika, Vol.28:2, P. 363, 1988

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The synthetic spectrum for the bright component of the close binary system υ Sgr in the wavelength region 3700 - 4800 Å was computed using the model atmosphere with the following parameters: Te = 13500K, lg g = 1.5 and N(H)/N(He) = 5×10-4. From the comparison of the observed and the synthetic spectrum in the wavelength region 3900 - 4900 Å the abundances of 33 chemical elements were estimated. The errors of the obtained abundances were discussed.

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