The K-correction For LMXBs. Application To X1822-371 and GX339-4
We present the K-correction for emission lines formed on the irradiated face of the companion stars in X-ray binaries. We compute this K-correction in a general approach as function of the mass ratio and the disc flaring angle. Our results combined with the detection of high energy emission lines arising from the donor star (e. g. Steeghs & Casares
Muñoz-Darias, T. et al.
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2006