Haniewicz, Henryk, Ferdman, Robert ORCID: https://orcid.org/0000-0002-2223-1235, Freire, P. C. C., Champion, D. J., Bunting, K. A., Lorimer, D. R. and McLaughlin, M. A. (2021) Precise mass measurements for the double neutron star system J1829+2456. Monthly Notices of the Royal Astronomical Society, 500 (4). pp. 4620-4627. ISSN 0035-8711
Full text not available from this repository.Abstract
PSR J1829+2456 is a radio pulsar in a relativistic binary system with another neutron star. It has a rotational period of 41 ms and a mildly eccentric (e = 0.14) 28 h orbit. We have continued its observations with the Arecibo radio telescope and have now measured the individual neutron star masses of this system: The pulsar and companion masses are 1.306 ± 0.007 M⊙ and 1.299 ± 0.007 M⊙ (2σ - 95 percent confidence, unless stated otherwise), respectively. We have also measured the proper motion for this system and used it to estimate a space velocity of 49+77-30 kms-1 with respect to the local standard of rest. The relatively low values for companion mass, space velocity, and orbital eccentricity in this system make it similar to other double neutron star systems in which the second-formed neutron star is thought to have formed in a low-kick, low mass-loss, symmetric supernova.
Item Type: | Article |
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Uncontrolled Keywords: | binaries: general,methods: observational,pulsars: general,astronomy and astrophysics,space and planetary science ,/dk/atira/pure/subjectarea/asjc/3100/3103 |
Faculty \ School: | Faculty of Science > School of Chemistry (former - to 2024) Faculty of Science > School of Physics (former - to 2024) |
UEA Research Groups: | Faculty of Science > Research Groups > Quantum Matter Faculty of Science > Research Groups > Numerical Simulation, Statistics & Data Science |
Related URLs: | |
Depositing User: | LivePure Connector |
Date Deposited: | 21 Apr 2021 23:48 |
Last Modified: | 07 Nov 2024 12:43 |
URI: | https://ueaeprints.uea.ac.uk/id/eprint/79842 |
DOI: | 10.1093/mnras/staa3466 |
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