Chandra Observations of the Young Pulsar PSR B0540–69

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© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation P. Kaaret et al 2001 ApJ 546 1159 DOI 10.1086/318287

0004-637X/546/2/1159

Abstract

The young pulsar PSR B0540-69 was one of the first targets observed with the Chandra X-Ray Observatory. The high angular resolution of Chandra allows us to resolve the compact nebula surrounding the pulsar. We have determined a position for PSR B0540-69 of R.A. = 05h40m11fs221,decl. = -69°19'54farcs98 (J2000) with a 1 σ radial uncertainty of 0farcs7. Combining our measurements of the pulsar period with previous measurements covering a span of 12 years, we derive a braking index of 2.082 ± 0.005 (95% confidence). The spectrum of the pulsed emission is consistent with a power law with a photon index of 1.83 ± 0.13. The compact nebula has a softer spectrum with a photon index of 1.85-2.26.

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10.1086/318287