Neutral hydrogen absorption towards G227.1 + 1.0

Details Neutral hydrogen absorption towards G227.1 + 1.0 Neutral hydrogen absorption towards G227.1 + 1.0

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.320...42g&link_type=abstract

Nature, Volume 320, Issue 6057, pp. 42-43 (1986).

Physics

8

Scientific paper

The radio source G227.1 + 1.0 (ref. 1) was observed in a search for young galactic supernova remnants, and its peculiar structure indicated that it might be a very young remnant. Chanan et al.2, however, have recently found a bright optical object with z = 0.073 close to the radio centre, which represents strong circumstantial evidence that the source is in fact a radio galaxy. Here we present a neutral hydrogen absorption profile observed with the Very Large Array (VLA) which confirms the extragalactic nature of this object.

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