The FAST Galactic Plane Pulsar Snapshot Survey. VIII. 116 Binary Pulsars

Abstract Finding pulsars in binaries is important for measurements of the masses of neutron stars (NSs), for tests of gravity theories, and for studies of star evolution. We are carrying out the Galactic Plane Pulsar Snapshot survey (GPPS) by using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Here we present the Keplerian parameters for 116 newly discovered pulsars in the FAST GPPS survey and obtain timing solutions for 29 pulsars. Companions of these pulsars are He white dwarfs (WDs), CO/ONe WDs, NSs, main sequence stars and ultra light objects or even planets. Our observations uncover eclipses of eight binary systems. The optical counterpart for the companion of PSR J1908+1036 is identified. The Post-Keplerian parameter <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>ω</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>̇</mml:mo> </mml:mrow> </mml:mover> </mml:math> for the double NS systems PSR J0528+3529 and J1844-0128 have been measured, with which the total masses of the binary systems are determined.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2024-12-27
DOI
https://doi.org/10.1088/1674-4527/ada3b8
Citations
18
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
5.97
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article

The FAST Galactic Plane Pulsar Snapshot Survey. VIII. 116 Binary Pulsars

J. L. Han, Z. L. Yang, Nan-Nan Cai, Jun Xu et al.
18 citations
Research in Astronomy and Astrophysics
Pulsars and Gravitational Waves Research
5.97
article

The FAST Galactic Plane Pulsar Snapshot Survey. VIII. 116 Binary Pulsars

J. L. Han, Z. L. Yang, Nan-Nan Cai, Jun Xu, D. J. Zhou, W. Q. Su, Chen Wang, W. C. Jing, Renxin Xu, Jianping Yuan, H. G. Wang, P F Wang, Tao Wang, Yi Yan, X. P. You
article en
18 citations

Abstract

Abstract Finding pulsars in binaries is important for measurements of the masses of neutron stars (NSs), for tests of gravity theories, and for studies of star evolution. We are carrying out the Galactic Plane Pulsar Snapshot survey (GPPS) by using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Here we present the Keplerian parameters for 116 newly discovered pulsars in the FAST GPPS survey and obtain timing solutions for 29 pulsars. Companions of these pulsars are He white dwarfs (WDs), CO/ONe WDs, NSs, main sequence stars and ultra light objects or even planets. Our observations uncover eclipses of eight binary systems. The optical counterpart for the companion of PSR J1908+1036 is identified. The Post-Keplerian parameter <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>ω</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>̇</mml:mo> </mml:mrow> </mml:mover> </mml:math> for the double NS systems PSR J0528+3529 and J1844-0128 have been measured, with which the total masses of the binary systems are determined.

Research in Astronomy and AstrophysicsVol. 25(1)
Southwest University (CN), Chinese Academy of Sciences (CN), Peking University (CN), Xinjiang Astronomical Observatory (CN), Guangzhou University (CN), Kavli Institute for Theoretical Sciences (CN), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN)
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
5.97
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