Timing and Precession of the Young, Relativistic Binary Pulsar PSR J1906+0746

TL;DR

This paper provides an updated timing analysis and profile evolution study of the young, relativistic binary pulsar PSR J1906+0746, revealing insights into its precession, beam shape, and companion characteristics.

Contribution

It offers the first comprehensive timing solution and profile evolution analysis, including precession and beam shape, for PSR J1906+0746, based on multi-telescope data.

Findings

Refined measurements of pulsar and companion masses.

Detection of profile evolution indicating precession.

Improved understanding of the pulsar's beam shape.

Abstract

We present an updated timing solution and an analysis of the profile evolution - including precession and beam shape - of the young, relativistic binary pulsar J1906+0746. The 144-ms pulsar, in a 3.98-hour orbit with eccentricity 0.085 (Lorimer et al. 2006), was initially discovered during the early stages of the ALFA (Arecibo L-band Feed Array) pulsar survey (Cordes et al. 2006) using the 305-metre Arecibo telescope and was subsequently found in archival Parkes Multibeam Survey data. We have since been regularly monitoring the system using the Arecibo and Green Bank telescopes, and include data from the Jodrell Bank, Parkes, Nancay and Westerbork telescopes. The nature of the binary companion will also be discussed based on improved estimates of the total and companion masses obtained from the updated timing solution.