NEUTRON STAR RADIUS MEASUREMENT WITH THE QUIESCENT LOW-MASS X-RAY BINARY U24 IN NGC 6397-Reference-Cited by-同舟云学术

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NEUTRON STAR RADIUS MEASUREMENT WITH THE QUIESCENT LOW-MASS X-RAY BINARY U24 IN NGC 6397

Published:2011-04-20 Issue:2 Volume:732 Page:88
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Guillot Sebastien,Rutledge Robert E.,Brown Edward F.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/732/i=2/a=88/pdf

Reference55 articles.

1. The fate of accreted CNO elements in neutron star atmospheres - X-ray bursts and gamma-ray lines

2. Variability in the Thermal Emission from Accreting Neutron Star Transients

3. Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars

4. MAPPING CRUSTAL HEATING WITH THE COOLING LIGHT CURVES OF QUASI-PERSISTENT TRANSIENTS

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2. Neutron stars in $$f(R,L_m,T)$$ gravity;The European Physical Journal C;2024-07-06

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4. Astrophysical Constraints on Dense Matter in Neutron Stars;Timing Neutron Stars: Pulsations, Oscillations and Explosions;2020-10-24

5. Spectral analysis of the quiescent low-mass X-ray binary in the globular cluster M30;Monthly Notices of the Royal Astronomical Society;2020-05-26

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