Hostname: page-component-6bf8c574d5-gr6zb Total loading time: 0 Render date: 2025-02-23T14:00:13.997Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Camilo, F. et al. 2002, ApJ, 571, L41.CrossRefGoogle Scholar
Losinskaya, T. A. 1986, Supernovae and Stellar Winds, (Moscow: Nauka)Google Scholar
Malofeev, V. M., Malov, O. I., & Glushak, A. P. 2001, IAU Circ. No. 7775.Google Scholar
Malofeev, V. M. et al. 2003, Astron. Reports, 47, 413.CrossRefGoogle Scholar
Malov, I. F. 1999, Astron. Reports, 43, 727.Google Scholar
Murray, S. et al. 2002, ApJ, 568, 226.CrossRefGoogle Scholar
Pacholczyk, A. G. 1970, Radio Astrophysics, (San Francisco: Freeman)Google Scholar
Williams, D. R. W. 1973, A&A, 28, 309.Google Scholar