most citedThe radial velocity curve for HeII emission cannot be used for component mass determination in SS433

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astro-ph.HE2025

Empirical correlation between masses of black holes and Wolf-Rayet stars derived from their mass distributions in spectroscopic binaries

Konstantin Postnov, Ivan Shaposhnikov, Anatol Cherepashchuk

We present observationally determined mass distributions of Wolf-Rayet (WR) stars in WR+OB binaries and black holes (BH) in spectroscopic binaries. Both WR and BH mass probability…