Radio maps revealing shell structures in five supernova remnants

Details Radio maps revealing shell structures in five supernova remnants Radio maps revealing shell structures in five supernova remnants

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..595c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, May 1983, p. 595-601.

Astronomy and Astrophysics

Astronomy

14

Astronomical Maps, Radio Astronomy, Stellar Envelopes, Supernova Remnants, Hydrogen Clouds, Milky Way Galaxy

Scientific paper

Five southern supernova remnants (SNRs) of small angular diameter (5-10 arcmin) have been mapped with the Fleurs synthesis telescope; at the resolution used (better than 1 arcmin) a shell structure can be seen in each remnant. One of the SNRs, G342.0-0.2, is a faint source which is confirmed as an SNR for the first time. This source and three others, G340.4 + 0.4, G340.6 + 0.3 and G341.9-0.3, lie close together on the sky; they have similar distance estimates of about 16 kpc and they all may be located in one of the spiral arms on the far side of the Galaxy. The fifth SNR, G352.7-0.1, although displaced from the others by more than 10 deg, is at a similar distance and is possibly in the same spiral arm.

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