2007
DOI: 10.1007/s10509-007-9330-1
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Spin-down of young pulsars with a fallback disk

Abstract: By performing Monte-Carlo calculations of the spin-down of young pulsars surrounded by a supernova fallback disk, we present possible constraints on the propeller torques exerted by the disks on neutron stars.

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“…From [151]. models, where LAT emission comes from late internal shocks [142,143,148,149]. The late internal shocks, however, can not explain temporally extended LAT emission which is apparently non-variabile.…”
Section: E Gev Emission and Plausible Interpretationsmentioning
confidence: 99%
“…From [151]. models, where LAT emission comes from late internal shocks [142,143,148,149]. The late internal shocks, however, can not explain temporally extended LAT emission which is apparently non-variabile.…”
Section: E Gev Emission and Plausible Interpretationsmentioning
confidence: 99%