Timing analysis of the core of the Crab-like SNR G21.5-0.9

Details Timing analysis of the core of the Crab-like SNR G21.5-0.9 Timing analysis of the core of the Crab-like SNR G21.5-0.9

2001-12-11

arxiv.org/abs/astro-ph/0112242v1

Astronomy and Astrophysics

Astrophysics

3 pages, latex, 2 tables, no figures, accepted for publication by A&A

Scientific paper

10.1051/0004-6361:20011839

The Crab-like SNR G21.5-0.9 was observed in the X-ray band (0.5-10 keV) by the XMM-Newton satellite for over 100 ks. The large effective area of the EPIC instrument has allowed us to to perform a deep search for pulsations from the central core of G21.5-0.9. No pulsations were found with upper limits on the pulsed fraction between 7.5 % and 40 % (depending on frequency and energy range).

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