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X-ray observations of the high magnetic field radio pulsar PSR J1814–1744

Published online by Cambridge University Press:  12 April 2016

M. J. Pivovaroff ,
V. M. Kaspi  and
F. Camilo
M. J. Pivovaroff
Affiliation:
MIT, Cambridge, MA 02139, USA
V. M. Kaspi
Affiliation:
MIT, Cambridge, MA 02139, USA
F. Camilo
Affiliation:
Columbia, U., New York, NY 10027, USA

Abstract

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We present X-ray observations of PSR J1814–1744, a 4 s radio pulsar with inferred surface dipole magnetic field strength 5.5 × 1013 G recently discovered in the on-going Parkes multibeam survey. This pulsar’s spin parameters are very similar to those of anomalous X-ray pulsars (AXPs). X-ray emission is not detected from the position of the radio pulsar in observations with ROSAT and ASCA. The derived upper flux limit implies an X-ray luminosity significantly smaller than those of all known AXPs. These results argue that magnetar mechanism invoked to explain X-ray emission from AXPs must depend on more than merely the inferred surface magnetic field strength as estimated from P and .

Type
Part 5. High-Energy Observations
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 349 - 350
Copyright
Copyright © Astronomical Society of the Pacific 2000

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