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The X-ray emission of the Crab-like pulsar PSR J0537-6910

T. Mineo·G. Cusumano·E. Massaro
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Abstract

In this paper we present some preliminary result on the spectral and timing analysis of the X-ray pulsed emission from the 16 ms pulsar PSR J0537-6910 in the energy range 0.1--30 keV, based on archival BeppoSAX and RossiXTE observations. This pulsar, discovered by Marshall et al.(1998) in the LMC field with RXTE, is the fastest spinning pulsar associated with a supernova remnant. It is characterized by strong glitch activity with the highest rate of all known Crab-like system.

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T. Mineo, G. Cusumano, E. Massaro. 2003-09-19. The X-ray emission of the Crab-like pulsar PSR J0537-6910. https://doi.org/10.1016/j.nuclphysbps.2004.04.110

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