2019 (v1)
Journal article
We consider a binary system composed of a pulsar and a massive, fast rotating, highly distorted main sequence star of mass M, spin angular momentum $\mathbf S $ , dimensionless mass quadrupole moment $J_2$ , equatorial and polar radii $R_\text {e},~R_\text {p}$ , flattening $\nu \doteq (R_\text {e}-R_\text {p})/R_\text {e}$ , and ellipticity...
Uploaded on: December 4, 2022