Radio tail source associated with NGC 7385

Details Radio tail source associated with NGC 7385 Radio tail source associated with NGC 7385

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....40..221s&link_type=abstract

Astronomy and Astrophysics, vol. 40, no. 1-2, Apr. 1975, p. 221-224.

Astronomy and Astrophysics

Astrophysics

34

Astronomical Maps, Galactic Structure, Radiant Flux Density, Radio Galaxies, Extragalactic Radio Sources, Galactic Clusters, Galactic Radiation, Microwave Emission

Scientific paper

Observations of 2247 + 11, a further example of the 'head-tail' class of radio source, are reported. The emission is associated with NGC 7385, a member of cluster Zwicky 2247.3 + 1107. The brightness distributions at 408 and 1415 MHz and the spectral index variations along the tail are discussed. Based on the magnetospheric model for radio tail sources of Jaffe and Perola, the density of the intracluster gas in this region is about 10 to the minus 27th gm per cu cm and its temperature is about one million K.

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