1. The FAST Galactic Plane Pulsar Snapshot Survey – V. PSR J1901+0658 in a double neutron star system.
- Author
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Su, W Q, Han, J L, Yang, Z L, Wang, P F, Yuan, J P, Wang, C, Zhou, D J, Wang, T, Yan, Y, Jing, W C, Cai, N N, Xie, L, Xu, J, Wang, H G, Xu, R X, and You, X P
- Subjects
NEUTRON stars ,BINARY stars ,PULSAR detection ,BINARY pulsars ,PULSARS ,ORBITS (Astronomy) - Abstract
Double neutron star (DNS) systems offer excellent opportunities to test gravity theories. We report the timing results of PSR J1901+0658, the first pulsar discovered in the FAST Galactic Plane Pulsar Snapshot (GPPS) Survey. Based on timing observations by FAST over 5 yr, we obtain the phase-coherent timing solution and derive the precise measurements of its position, spin parameters, orbital parameters, and dispersion measure. It has a period of 75.7 ms, a period derivative of 2.169(6) × 10
−19 s s−1 , and a characteristic age of 5.5 Gyr. This pulsar is in an orbit with a period of 14.45 d and an eccentricity of 0.366. One post-Keplerian parameter, periastron advance, has been well-measured as being 0.00531(9) deg yr−1 , from which the total mass of this system is derived to be 2.79(7) M⊙ . The pulsar has the mass upper limit of 1.68 M⊙ , so the lower limit for the companion mass is 1.11 M⊙ . Because PSR J1901+0658 is a partially recycled pulsar in an eccentric binary orbit with such a large companion mass, it should be in a DNS system according to the evolution history of the binary system. [ABSTRACT FROM AUTHOR]- Published
- 2024
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