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- W63940930 abstract "Hydrogen and helium accreted onto a neutron star undergo thermonuclear burning. Explosive burning is observed as a type I X-ray burst. We describe the different burning regimes and focus on some of the current inconsistencies between theory and observations. Of special interest are the rare kinds of X-ray bursts such as carbon-fueled superbursts and helium-fueled intermediately long X-ray bursts. These bursts are thought to originate deeper in the neutron star envelope, such that they are probes of the thermal properties of the crust. We investigate the possibility of observing superbursts with the wide-field instruments INTEGRAL-ISGRI and Swift-BAT. We find that only the brightest bursts are detectable." @default.
- W63940930 created "2016-06-24" @default.
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- W63940930 date "2008-11-27" @default.
- W63940930 modified "2023-09-26" @default.
- W63940930 title "On burning regimes and long duration X-ray bursts" @default.
- W63940930 cites W2128326290 @default.
- W63940930 doi "https://doi.org/10.48550/arxiv.0811.4574" @default.
- W63940930 hasPublicationYear "2008" @default.
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