... Next: Change of Binary Parameters: Up: Evolutionary Scenarios of Binary Previous: Wolf-Rayet and He stars . ... When a massive star becomes a Wolf-Rayetstar, its stellar wind can significantly increase (up to yr ). ...
... 1993)[ 31 ], so AIC BH with masses close to the OV-limit in circular orbits around the remaining star core (a Wolf-Rayetstar (WR) or a white dwarf (WD)) will form, unless the spiral-in ends by coalescence of the compact star with the stellar core and ...
... main sequence, red (super)giant, helium (Wolf-Rayet) star, hot WD), in which stellar parameters significantly differ from ... Roche lobe overflow (stage III) . Wolf-Rayet and He stars (stage IV) . Stellar Winds From Normal Stars . ...
... From the point of view of NS evolution in massive binary systems, identification of the X-ray source Cyg X-3 as a Wolf-Rayetstar is of great significance (van Kerkwijk et al. ...
... Next: Wolf-Rayet and He stars Up: Principal Evolutionary States of Previous: Post main sequence stars . ... Next: Wolf-Rayet and He stars Up: Principal Evolutionary States of Previous: Post main sequence stars Mike E. Prokhorov . ...