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°, 4500° and 5000° and for hydrogen-to-metal ratios of 1, 102, 103 and 104 times the solar values, and for surface gravities of 2×104 and 2×102. The effect of metal deficiency on the atmospheric structure of these stars are studied.

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