Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars
arXiv:astro-ph/0411207
Abstract
We summarize constraints on neutron star masses from ongoing timing observations of pulsar-white dwarf binaries at Arecibo. The trend is toward pulsar masses larger than the canonical value of 1.35 solar masses.
2 pages, to appear in "Binary Radio Pulsars", eds F. A. Rasio & I. H. Stairs, PASP conf series