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Chemical Abundances in the Secondary Star in the Black Hole Binary A0620โˆ’00

Chemical Abundances in the Secondary Star in the Black Hole Binary A0620โˆ’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 chi^2 minimization procedure to explore a grid of 800 000 LTE synthetic spectra computed โ€ฆ