Chemical Abundances in the Secondary Star in the Black Hole Binary A0620-00
Using a high-resolution spectrum of the secondary star in the black hole binary A0620-00, we have derived the stellar parameters and veiling caused by the accretion disk in a consistent way. We have used a χ2 minimization procedure to explore a grid of 800,000 LTE synthetic spectra computed for a plausible range of both stellar and veiling
González Hernández, Jonay I. et al.
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2004