Very high resolution observations of the radio source in the supernova remnant G127.1+0.5

Details Very high resolution observations of the radio source in the supernova remnant G127.1+0.5 Very high resolution observations of the radio source in the supernova remnant G127.1+0.5

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...260l..69g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 260, Sept. 15, 1982, p. L69-L73.

Astronomy and Astrophysics

Astronomy

14

Radio Sources (Astronomy), Supernova Remnants, Very Long Base Interferometry, Astronomical Maps, Brightness Distribution, High Resolution, Plasma Jets, Stellar Envelopes

Scientific paper

The results of recent very long baseline interferometry of G127.11+0.54 at 10.65 GHz reveal a core dual 'jet' structure. The morphology and physical properties of the compact source are similar to those of SS 433. The combined data from various studies of this object suggest that G127.11+0.54 may be the stellar remnant of the supernova event which also produced the supernova remnant G127.1+0.5.

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