... The Evolutionary Evidence for Most Be Stars Being Paired with Hot White Dwarfs", Natalya V. Raguzova, The Be Phenomenon in Early-Type Stars, IAU Colloquium 175, ASP Conference Proceedings, Vol. 214, edited by Myron A. Smith and Huib F. Henrichs. ...
... in a binary is treated as an instantaneous mass loss of the exploding star ... kick velocity is imparted to young neutron stars due to possible asymmetry of the ... the changing mass of the exploding star is calculated and kick vwlocity arbitrarily ...
... The states of stars and binary parameters at the beginning of a stage fully determine the fate of the binary to the end of the stage, under the assumption that the parameters of the surrounding plasma each star provides for its companion remain unchanged ...
... Then we normalized the figures so as to be in agreement with the Tamblyn & Rieke (1993) calculations of the number of massive OB-stars (1,900 stars with ) that survived Myrs after the starburst onset (this age is supported below by an additional argument ...
... semi-major axis a ) with a normal star losing matter in the form of stellar wind ... the stellar wind velocity of hot stars are connected through the empirical relation ...
... rates of compact binaries (double neutron stars or black holes) are calculated based ... 10-700 black holes and only 1 neutron star coalescences in a 1-year integration time ... BH+BH merging . Parameters of binary compact star evolution . ...
... star may trap a considerable part of the relativistic wind ( , where is the radius ... star and nuclear transformation of ultrahigh-energy particles colliding with the ... star must be strictly periodic in nature due to the rotation of a normal star ...