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

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

2003-09-19

arxiv.org/abs/astro-ph/0309523v1

Nucl.Phys.Proc.Suppl.132:632-635,2004

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures. Contribution to the proceedings of "The Restless High-Energy Universe", Amsterdam, May 5-8, 2003. Editors:

Scientific paper

10.1016/j.nuclphysbps.2004.04.11

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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