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Accreting, Mixing, and X-ray Bursting
AIP Conference Proceedings, 2008During accretion, a neutron star (NS) is spun up as angular momentum is transported through its liquid surface layers. We study the resulting differentially rotating profile, focusing on the impact this has for type I X‐ray bursts. The viscous heating is found to be negligible, but turbulent mixing can be activated.
Anthony L. Piro +5 more
openaire +1 more source
A Roadmap to Gamma-Ray Bursts: New Developments and Applications to Cosmology
Galaxies, 2021Orlando Luongo +2 more
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Gamma-Ray Bursts at TeV Energies: Observational Status
Galaxies, 2022Koji Noda, Robert Parsons, Noda Koji
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Distinction of groups of gamma-ray bursts in the BATSE catalog through fuzzy clustering
Astronomy and Computing, 2021Soumita Modak
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The Ep,i–Eiso correlation: type I gamma-ray bursts and the new classification method
Monthly Notices of the Royal Astronomical Society, 2020Pavel Minaev +2 more
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Stripping Model for Short Gamma-Ray Bursts in Neutron Star Mergers
Particles, 2022Sergei Blinnikov, Nikita Kramarev
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Synchrotron self-compton emission in the two-component jet model for gamma-ray bursts
Journal of High Energy Astrophysics, 2023Ryo Yamazaki +2 more
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High-redshift long gamma-ray bursts Hubble diagram as a test of basic cosmological relations
Monthly Notices of the Royal Astronomical Society, 2020Lorenzo Amati +2 more
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