... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...

arxiv:1410.4898 PSR J1738+0333: первый миллисекундный пульсар в паре с пульсирующим белым карликом (PSR J1738+0333: The First Millisecond Pulsar + Pulsating White Dwarf Binary) . ... arxiv:1410.4250 Масса менее 15 солнечных у черной дыры в ультрамощном источнике (A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source) . ... What would a binary black hole merger look like?) ... обзор arxiv:1410.6865 Лунные ресурсы: обзор (Lunar Resources: A Review) . ...

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