Different Accretion Heating of the Neutron Star Crust during Multiple Outbursts in MAXI J0556–332
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/aa9e03/pdf
Reference36 articles.
1. Variability in the Thermal Emission from Accreting Neutron Star Transients
2. MAPPING CRUSTAL HEATING WITH THE COOLING LIGHT CURVES OF QUASI-PERSISTENT TRANSIENTS
3. The Swift X-Ray Telescope
4. Cooling of the Crust in the Neutron Star Low-Mass X-Ray Binary MXB 1659-29
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1. Neutron-star measurements in the multi-messenger Era;Astroparticle Physics;2024-06
2. A “Hyperburst” in the MAXI J0556–332 Neutron Star: Evidence for a New Type of Thermonuclear Explosion;The Astrophysical Journal;2022-07-01
3. Crust Cooling of Soft X-Ray Transients—the Uncertainties of Shallow Heating;Research in Astronomy and Astrophysics;2022-04-29
4. Improved nuclear physics near A=61 refines urca neutrino luminosities in accreted neutron star crusts;Physical Review C;2022-02-18
5. Constraining the properties of dense neutron star cores: the case of the low-mass X-ray binary HETE J1900.1–2455;Monthly Notices of the Royal Astronomical Society;2021-08-04
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