ar X iv : a st ro - p h / 03 09 52 3 v 1 1 9 Se p 20 03 1 The X - ray emission of the Crab - like pulsar PSR J 0537 − 6910
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چکیده
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. [1] 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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تاریخ انتشار 2003