On the Mass and Inclination of the PSR J2019+2425 Binary System

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Abstract
We report on 9 years of timing observations of PSR J2019+2425, a millisecond pulsar in a wide 76.5 day orbit with a white dwarf. We measure a significant change over time of the projected semimajor axis of the orbit, /x = × 10-15 s-1, where x ≡ (a1 sin i)/c. We attribute this to the proper motion of the binary. This constrains the inclination angle to i < 72°, with a median likelihood value of 63°. A similar limit on the inclination angle arises from the lack of a detectable Shapiro delay signal. These limits on inclination angle, combined with a model of the evolution of the system, imply that the neutron star mass is at most 1.51 M☉; the median likelihood value is 1.33 M☉. In addition to these timing results, we present a polarization profile of this source. Fits of the linear polarization position angle to the rotating vector model indicate that the magnetic axis is close to alignment with the rotation axis, α < 30°.
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