Abstract
Interpretation of X-ray eclipses in SS 433 binary system in the framework of wind-wind collision model yields high value of mass ratioq =m x /m v > 1 which implies high mass of relativistic objectm x > 8M ⊙ .
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Cherepashchuk, A.M., Bychkov, K.V. & Seifina, E.V. Colliding winds model of X-ray radiation in SS 433: analysis of X-ray eclipses. Astrophys Space Sci 229, 33–48 (1995). https://doi.org/10.1007/BF00658564
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DOI: https://doi.org/10.1007/BF00658564