Implications of PSR J0737-3039B for the Galactic NS-NS binary merger rate

Authors

C. Kim
B. B. P. Perera
M. A. McLaughlin

Author ORCID Identifier

N/A

https://orcid.org/0000-0002-8509-5947

https://orcid.org/0000-0001-7697-7422

Document Type

Article

Publication Date

2015

Abstract

The Double Pulsar (PSR J0737−3039) is the only neutron star–neutron star (NS–NS) binary in which both NSs have been detectable as radio pulsars. The Double Pulsar has been assumed to dominate the Galactic NS–NS binary merger rate

Digital Commons Citation

Kim, C.; Perera, B. B. P.; and McLaughlin, M. A., "Implications of PSR J0737-3039B for the Galactic NS-NS binary merger rate" (2015). Faculty & Staff Scholarship. 191.
https://researchrepository.wvu.edu/faculty_publications/191

Source Citation

Kim, C.., Perera, B. B. P.., & McLaughlin, M. A.. (2015). Implications Of Psr J0737-3039B For The Galactic Ns-Ns Binary Merger Rate. Monthly Notices of the Royal Astronomical Society, 448(1), 928-938. http://doi.org/10.1093/mnras/stu2729