A study of the Crab Nebula at 2.7 GHz with an angular resolution 3.7 X 10 arcsec. I - The observations

Details A study of the Crab Nebula at 2.7 GHz with an angular resolution 3.7 X 10 arcsec. I - The observations A study of the Crab Nebula at 2.7 GHz with an angular resolution 3.7 X 10 arcsec. I - The observations

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..775s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Mar. 1979, p. 775-778. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

24

Astronomical Photography, Crab Nebula, Radio Astronomy, Circular Polarization, Filaments, Linear Polarization, Pulsars

Scientific paper

The Crab Nebula has been observed with the Cambridge 5-km radio telescope at a frequency of 2.695 GHz, giving an angular resolution of 3.7 x 10 arcsec. Maps are presented showing total intensity and linear polarization. The nebula has a filamentary structure at this wavelength, strikingly similar to that seen in optical line emission. An upper limit of 0.1 percent is placed on any circular polarization.

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