The radio halos of pulsars

Details The radio halos of pulsars The radio halos of pulsars

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..324g&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, Mar.-Apr. 1981, p. 324-333. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Halos, Pulsars, Radio Sources (Astronomy), Radio Spectra, Electron Emission, Interstellar Magnetic Fields, Nonthermal Radiation, Radio Telescopes, Relativistic Particles, Supernova Remnants, Synchrotron Radiation

Scientific paper

The results of a search for radio halos of 22 pulsars at a frequency of 102 MHz are reported. Sources of continuous radio emission G228.9+43.7, G55.7+3.4, and G98.4-76 were detected in the direction of the pulsars 0950+08, 1919+21, and 2217+47, respectively. The radio source G228+43.7 has been found to be a pulsar radio halo; the spectral index of this source is 2 + or - 1; the nonthermal spectrum is explained by synchrotron radiation from relativistic electrons injected by the pulsar in magnetic fields of pulsar origin. It is shown that a commonly used radio-halo model, based on synchrotron radiation from relativistic electrons in interstellar magnetic fields, is unacceptable. Finally, it is noted that the nonthermal radio source G98.4-7.6 can be interpreted as a radio halo of the pulsar 2217+47 or a supernova remnant.

Affiliated with

Also associated with

No associations

Rating

The radio halos of pulsars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The radio halos of pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The radio halos of pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-782004