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An extremely bright gamma-ray pulsar in the Large Magellanic Cloud

Author(s)
Fermi LAT Collaboration
Ackermann, M.
Albert, A.
Ciprini, Stefano  
Cutini, Sara
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Date Issued
2015-11-01
Mission(s)
Fermi  
Abstract
Pulsars are rapidly spinning, highly magnetized neutron stars, created in the gravitational collapse of massive stars. We report the detection of pulsed giga--electron volt gamma rays from the young pulsar PSR J0540--6919 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This is the first gamma-ray pulsar detected in another galaxy. It has the most luminous pulsed gamma-ray emission yet observed, exceeding the Crab pulsar's by a factor of 20. PSR J0540--6919 presents an extreme test case for understanding the structure and evolution of neutron star magnetospheres.
URI
https://hdl.handle.net/20.500.13025/4303
DOI
10.1126/science.aac7400
URL
http://adsabs.harvard.edu/abs/2015Sci...350..801F
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