A new simulation of the evolution of binary stars shows that previously neglected millisecond pulsars could explain the excess gamma-ray radiation seen in our Galaxy’s center.
With the H.E.S.S. observatory and the Fermi satellite, researchers track the eruption of RS Ophiuchi. For the first time, it has been possible to observe the outburst of a nova in very high-energy gamma light and to follow the glow and subsequent.
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