The nature of the central source of the supernova remnant G 179.0 + 2.7

Details The nature of the central source of the supernova remnant G 179.0 + 2.7 The nature of the central source of the supernova remnant G 179.0 + 2.7

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223...66f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 66-70.

Astronomy and Astrophysics

Astrophysics

3

Elliptical Galaxies, Radio Galaxies, Supernova Remnants, Absorption Spectra, Ionized Gases, Radio Emission, Very Large Array (Vla)

Scientific paper

The triple radio source located towards the center of the supernova remnant G 179.0 + 2.7 was observed at 1.49 and 4.86 GHz with high angular resolution with the VLA. The source is identified as a double-sided radio galaxy unrelated to the supernova remnant. Optical observations with a 3.5-m telescope reveal the associated elliptical galaxy of magnitude 17 + or - 1 mag at a distance of 180 Mpc (H0) = 50 km/s Mpc).

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