A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy-Reference-Cited by-同舟云学术

A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

Published:2021-09-01 Issue:2 Volume:918 Page:L27
ISSN:2041-8205
Container-title:The Astrophysical Journal Letters
language:
Short-container-title:ApJL

Author:

Riley Thomas E.^ORCID,Watts Anna L.^ORCID,Ray Paul S.^ORCID,Bogdanov Slavko^ORCID,Guillot Sebastien^ORCID,Morsink Sharon M.^ORCID,Bilous Anna V.^ORCID,Arzoumanian Zaven,Choudhury Devarshi^ORCID,Deneva Julia S.^ORCID,Gendreau Keith C.^ORCID,Harding Alice K.^ORCID,Ho Wynn C. G.^ORCID,Lattimer James M.^ORCID,Loewenstein Michael,Ludlam Renee M.^ORCID,Markwardt Craig B.^ORCID,Okajima Takashi^ORCID,Prescod-Weinstein Chanda^ORCID,Remillard Ronald A.^ORCID,Wolff Michael T.^ORCID,Fonseca Emmanuel^ORCID,Cromartie H. Thankful^ORCID,Kerr Matthew^ORCID,Pennucci Timothy T.^ORCID,Parthasarathy Aditya^ORCID,Ransom Scott^ORCID,Stairs Ingrid^ORCID,Guillemot Lucas^ORCID,Cognard Ismael^ORCID

Funder

EC ∣ European Research Council

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ac0a81/pdf

Reference148 articles.

1. GW170817: Measurements of Neutron Star Radii and Equation of State

2. Properties of the Binary Neutron Star Merger GW170817

3. GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object