Constraining the mass and radius of neutron stars in globular clusters

Author:

Steiner A W12,Heinke C O3,Bogdanov S4,Li C K35,Ho W C G6ORCID,Bahramian A37ORCID,Han S1

Affiliation:

1. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA

2. Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA

3. Department of Physics, University of Alberta, CCIS 4-183, Edmonton AB T6G 2E1, Canada

4. Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA

5. Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, 100049 Beijing, PR China

6. Mathematical Sciences, Physics and Astronomy and STAG Research Centre, University of Southampton, Southampton SO17 1BJ, UK

7. Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA

Funder

NSF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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