Spectroscopic modelling of two high-mass X-ray binaries, Cyg X–3 and 4U 1538–522
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DOI: 10.1093/mnras/stab2231
Abstract: We report a detailed modelling of soft X-ray emission lines from two stellar wind-fed Galactic high-mass X-ray binary (HMXB) systems, Cyg X-3 and 4U 1538-522, and estimate physical parameters, e.g. hydrogen density, radiation field, chemical… read more here.
Keywords: field; mass ray; cyg 1538; high mass ... See more keywords