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The Radio Pulsar J0205+6449 in the SNR 3C 58

Published online by Cambridge University Press:  19 July 2016

V. M. Malofeev ,
I. F. Malov ,
O. I. Malov  and
A. P. Glushak
V. M. Malofeev
Affiliation:
Lebedev Physical Institute, Moscow, Russia
I. F. Malov
Affiliation:
Lebedev Physical Institute, Moscow, Russia
O. I. Malov
Affiliation:
Lebedev Physical Institute, Moscow, Russia
A. P. Glushak
Affiliation:
Lebedev Physical Institute, Moscow, Russia

Abstract

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Pulsed radio emission has been detected from the X-ray pulsar J0205+6449 in the SNR 3C 58 at 111 and 88 MHz on radio telescopes of the Pushchino Radio Astronomy Observatory. The dispersion measure DM = 141 pc cm−3 has been confirmed. The synchrotron mechanism is proposed for the radio and X-ray emission to explain the lower X-ray and radio luminosities of this pulsar compared to the Crab pulsar.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 443 - 444
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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