• Corpus ID: 119041756

The orientation and magnitude of the orbital precession velocity of a binary pulsar system with double spins

@inproceedings{BPGong2003TheOA,
  title={The orientation and magnitude of the orbital precession velocity of a binary pulsar system with double spins},
  author={B.P.Gong},
  year={2003}
}
The measurability of the spin--orbit (S--L) coupling induced orbital effect is dependent on the orientation and magnitude of the orbital precession velocity, ${\bf \Omega}_0$. This paper derives ${\bf \Omega}_0$ in the case that both spins in the binary system contribute to the spin--orbit (S--L) coupling, which is suitable for the most popular binary pulsars, Neutron star--White Dwarf star (NS--WD) binaries (as well as for NS--NS binaries). This paper shows that from two constraints, the…