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Spectral analysis of young gamma-ray pulsars with Fermi

โœ Scribed by Fabio Gargano


Publisher
Elsevier Science
Year
2011
Tongue
English
Weight
305 KB
Volume
630
Category
Article
ISSN
0168-9002

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The Crab Pulsar is a relatively young neutron star. The Pulsar is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was observed on Earth in the year 1054. The Crab Pulsar has been extensively observed in the gamma-ray energy band by the Large Area Telescope (LAT), the m