Lunar occultation observations of 15 Abell clusters at 327 MHz

Details Lunar occultation observations of 15 Abell clusters at 327 MHz Lunar occultation observations of 15 Abell clusters at 327 MHz

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191..581s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, May 1980, p. 581-587. Research supported by the Alexander von Humb

Astronomy and Astrophysics

Astronomy

4

Galactic Clusters, Lunar Occultation, Microwave Emission, Millimeter Waves, Radio Sources (Astronomy), High Resolution, Luminous Intensity, Quasars, X Ray Sources

Scientific paper

The results of high-resolution, metre-wavelength observations, together with optical identification data, are presented for 17 discrete sources that dominate the radio emission form the direction of 15 Abell clusters. With only two exceptions, all the sources have been resolved. The sample contains two head-tail sources, including that in the X-ray emitting cluster Abell 401. The spectral indices of both the head and tail components of this source are found to be approximately 0.8 and the size of its tail exhibits no strong dependence on the observing frequency.

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