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Discovery of Extreme, Roughly-Daily Superflares on the Recurrent Nova V2487 Oph

publication date21. 01. 2022
tag iconNova Stars White dwarf

Nova V2487 Oph, spectral distribution

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X-ray detection of a nova in the fireball phase

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A Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc

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Localized thermonuclear bursts from accreting magnetic white dwarfs

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Repeating nova RS Ophiuchi generated gamma radiation for a month after its latest explosion

Astronomers detected gamma radiation coming from the binary system RS Ophiuchi for a month after the thermonuclear explosion. This star system contains a small white dwarf and a red giant. According to a new study the radiation was emitted from winds of the secondary red giant star accelerated by the nova explosion.

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