Detection of Fine Structure in the Crab Nebula at 38 Mc/s

Details Detection of Fine Structure in the Crab Nebula at 38 Mc/s Detection of Fine Structure in the Crab Nebula at 38 Mc/s

Jul 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.203..171h&link_type=abstract

Nature, Volume 203, Issue 4941, pp. 171 (1964).

Physics

23

Scientific paper

SEVERAL observations of the distribution of radio brightness across the Crab Nebula have been reported over a wide range of frequencies1,2,4-6. The results indicate that the distribution, while slightly elongated, has an approximately Gaussian profile. There is some evidence that the angular diameter increases at the lowest frequencies1, but no fine structure has been detected. Kuz'min and Salamonovich6, observing at a wave-length of 8 mm, noted a small source slightly displaced from the centre of the nebula which they ascribed to an independent source of thermal origin.

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