... The Effect of Relativistic Wind on Accretion Flow Parameters. ... due to the fact that the power of a pulsar, and hence the pressure of the pulsar wind, depends very strongly on its period (as ...
... The Radiopulsar PSRB1259-63 - a Probe in the Stellar Wind Plasma. ... confirming the theory of evolution of NS, but also for understanding processes occurring in stellar winds from normal stars ...
... Determination of the stellar wind velocity.. ... So we can evaluate v (in this case it is the stellar wind velocity, ): . Values of are shown in table 3. Sergei B. Popov . ...
... a ) with a normal star losing matter in the form of stellar wind (with a loss rate ... outflow rate, luminosity and the stellar wind velocity of hot stars are connected ... a NS, assuming that the relativistic wind ejected by the star is spherically ...
... to form NS of 1.4 M; when a BH with a mass of is formed, where is either the mass of the pre-collapsing star (in the case of low stellar wind mass-loss scenario), or the initial mass of the star (in teh case of the high stellar wind mass-loss scenario ...
... Next: Mass change Up: Evolutionary Scenarios of Binary Previous: Stellar Winds From Normal . ... star should change (if at all) (e.g. due to stellar wind or RL overflow), that is we know the quantity the leading (faster ...
... Using strong dependence of D on the velocity for Vela X-1 and GX 301-2, systems accreting from a stellar wind, we determined the stellar wind velocity. ...
... Wolf-Rayet and He stars (stage IV) . Stellar Winds From Normal Stars . ... The Effect of Relativistic Wind on Accretion Flow Parameters . ... The Radiopulsar PSRB1259-63 - a Probe in the Stellar Wind Plasma . ...