Atmospheres of Extreme Metal-Deficient Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Atmospheric models have been constructed for effective temperatures
4000°, 45000 and 50000 and for hydrogen-to-metal ratios of 1, 102,
1O~ and 10~ times the solar values, and for surface gravities of 2 x 1O~
and 2 x 102. The effect of metal deficiency on the atmospheric structure
of these stars are studied

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