EVIDENCE OF AN ASTEROID ENCOUNTERING A PULSAR
Debris disks and asteroid belts are expected to form around young pulsars due to fallback material from their original supernova explosions. Disk material may migrate inward and interact with a pulsar's magnetosphere, causing changes in torque and emission. Long-term monitoring of PSR J0738-404...
Huvudupphovsmän: | Brook, P, Karastergiou, A, Buchner, S, Roberts, S, Keith, M, Johnston, S, Shannon, R |
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Materialtyp: | Journal article |
Språk: | English |
Publicerad: |
2014
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