Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars

Details Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars

2004-11-08

arxiv.org/abs/astro-ph/0411207v1

Astronomy and Astrophysics

Astrophysics

2 pages, to appear in "Binary Radio Pulsars", eds F. A. Rasio & I. H. Stairs, PASP conf series

Scientific paper

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.

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