XMM-Newton observations of a sample of radio pulsars

Details XMM-Newton observations of a sample of radio pulsars XMM-Newton observations of a sample of radio pulsars

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nuphs.132..636o&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 132, p. 636-639.

Physics

Nuclear Physics

Scientific paper

Results of a search for X-ray counterparts of radio pulsars with the EPIC-PN instrument on board XMM-Newton are presented. Despite the mostly relatively short exposure times (<8 ks, PSR B0823+26 was observed for 50 ks) these observations have resulted in much improved upper limits over previous work and, in the case of PSR B1719-37, a first detection in X-rays. The obtained upper limits and detection are found to be consistent with the empirical relation as found by Verbunt et al. and Becker & Trümper.

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