Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star-Reference-Cited by-同舟云学术

Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star

Published:2019-12-12 Issue:1 Volume:887 Page:L26
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bogdanov Slavko^ORCID,Lamb Frederick K.^ORCID,Mahmoodifar Simin^ORCID,Miller M. Coleman^ORCID,Morsink Sharon M.^ORCID,Riley Thomas E.^ORCID,Strohmayer Tod E.^ORCID,Tung Albert K.,Watts Anna L.^ORCID,Dittmann Alexander J.,Chakrabarty Deepto^ORCID,Guillot Sebastien^ORCID,Arzoumanian Zaven,Gendreau Keith C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab5968/pdf

Reference70 articles.

1. Equation of state of nucleon matter and neutron star structure

2. UNIVERSALITY OF THE ACCELERATION DUE TO GRAVITY ON THE SURFACE OF A RAPIDLY ROTATING NEUTRON STAR

3. Testing the rotating hotspot model using X-ray burst oscillations from 4U 1636−536

4. EFFECTS OF SPOT SIZE ON NEUTRON-STAR RADIUS MEASUREMENTS FROM PULSE PROFILES

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