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Nachrichten, Termine, Experten
Nachrichten, Termine, Experten
Abb. 1: Künstlerische Darstellung der im Röntgenlicht leuchtenden Magnetosphäre eines Millionen Jahre alten Pulsars. Der Neutronenstern selbst ist unsichtbar, da seine Oberfläche nicht mehr genügend Hitze besitzt, um Röntgenstrahlung zu emittieren. Oberhalb der beiden magnetischen Pole werden elektrisch geladene Teilchen aus der Magnetosphäre nach außen beschleunigt - und senden dabei intensive, stark gerichtete Strahlung aus, die sich mit XMM-Newton beobachten lässt.
Source: Bild: Werner Becker / MPI für extraterrestrische Physik
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