G70.68 + 1.20 - A thermal source, not a supernova remnant

Details G70.68 + 1.20 - A thermal source, not a supernova remnant G70.68 + 1.20 - A thermal source, not a supernova remnant

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.219p..39g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 219, April 1, 1986, p. 39P-43P.

Astronomy and Astrophysics

Astronomy

15

Milky Way Galaxy, Radio Sources (Astronomy), Stellar Envelopes, Stellar Spectrophotometry, Supernova Remnants, Thermal Emission, Radiant Flux Density, Spectral Resolution

Scientific paper

G70.68+1.20 is a small shell source, ≡20 arcsec in extent, which has recently been proposed as a very young galactic supernova remnant. 5-GHz observations with the 5-km telescope at a resolution of ≡2×4 arcsec2 (RA×Dec) are presented, and discussed together with other radio, optical and IR data. These favour the interpretation that the source is thermal, rather than a young supernova remnant.

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