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Binary evolution and formation of binary millisecond pulsars.
1994The high incidence of binaries among millisecond pulsars in combination with rapid spin and relatively weak magnetic fields strongly suggest a large fraction of them (if not all) are old neutron stars that have been 'recycled' by accretion of mass and angular momentum from a companion star (Bhattacharya and van den Heuvel, 1991, Phys. Rep., 203, 1). We
openaire +2 more sources
Formation and evolution of binary and millisecond radio pulsars
Physics Reports, 1991Dipankar Bhattacharya +1 more
exaly
Bounding the mass of graviton in a dynamic regime with binary pulsars
Physical Review D, 2019Lijing Shao, Bo-Qiang Ma, Xueli Miao
exaly
Determination of the orbital parameters of binary pulsars
Monthly Notices of the Royal Astronomical Society, 2008Nityananda Rajaram
exaly
Discovery of four binary millisecond pulsars
Monthly Notices of the Royal Astronomical Society, 1996Benjamin Stappers +2 more
exaly
Interstellar scintillations of binary pulsars
AIP Conference Proceedings, 1988Cordes J M, Wolszczan A, Weisberg J M
exaly

