High Resolution Map of NGC1265

Details High Resolution Map of NGC1265 High Resolution Map of NGC1265

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.244..502w&link_type=abstract

Nature, Volume 244, Issue 5417, pp. 502-504 (1973).

Physics

39

Scientific paper

THE radio sources associated with NGC1265 and IC310 have ``head-tail'' structures with the heads coinciding with the optical galaxies1. Ryle and Windram suggested1 that both radio sources were ignited by a relativistic particle wind from the nearby Seyfert galaxy NGC1275. Hill and Longair2 drew attention to further examples of galaxies in clusters with the same peculiar radio morphology.

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