Detection of change in rotation measure of the VELA pulsar

Details Detection of change in rotation measure of the VELA pulsar Detection of change in rotation measure of the VELA pulsar

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.265..224h&link_type=abstract

Nature, vol. 265, Jan. 20, 1977, p. 224, 225.

Physics

13

Pulsars, Stellar Magnetic Fields, Stellar Rotation, Supernova Remnants, Faraday Effect, Field Strength, Filaments, Frequency Response

Scientific paper

Observations of PSR 0833-45 at well separated frequencies on three occasions are reported. The observations permitted accurate determinations of the rotation measure along the path to the source and of the position angle of the emitted radiation extrapolated to infinite frequency, the intrinsic position angle. The data show that there has been a significant chance in the rotation measure along the path to the source during the past 6 years. Possible reasons for this change are discussed.

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