... star to the class of massive binaries if the primary component mass is large ... star (i.e. during Roche lobe overflow), the probability of such collapse being ... pulsar in a pair with a helium star (WR-star in the case of massive binaries ...
... As is seen in Fig. , the old galactic neutron stars fill a thorus-like region extended up tens kiloparsecs above the galactic plane with sharp deficiency of stars toward the galactic axis. ...
... The mass of the star that loses matter is . ... Accordingly, the mass of the accreting star is . ... At stages with RL overflow and both normal stars we will assume a mildly non ...
... Next: Initial conditions Up: Old neutron star distribution Previous: Introduction . ... to find stationary space distribution of stars which have had certain initial space ...
... The magnetosphere of the star represents an obstacle for the flow, and a shock wave stands in front of the star. ... Results of our simulations may be applied to other strongly magnetized stars, for example, white dwarfs and magnetic Ap stars.. ...
... Binary Star . Binary System of X-ray Pulsar . ... Binary System of X-ray Pulsar . Disk Accretion onto Magnetized Neutron Star . ... Interchange Instability in the Accretion Disk around Neutron Stars . ...