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- W1988744333 abstract "Discrete sources in the southern spiral arm of M 33 have been observed with the Westerbork Synthesis Radio Telescope at 49 and 21 cm and the Very Large Array at 6 cm. The three optically confirmed supernova remnants were detected with the WSRT and were found to have non-thermal spectral indices. Two of these SNR were detected with the VLA with a resolution of ∼ 1.5 arcsec (5 pc). If it is assumed that these M33 SNR are similar to galactic SNR, the surface-brightness–diameter relationship proposed by Caswell & Lerche (1979) indicates a distance of 860 ± 200 kpc for M33." @default.
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- W1988744333 date "1980-12-01" @default.
- W1988744333 modified "2023-09-28" @default.
- W1988744333 title "Radio observations of three supernova remnants in M33" @default.
- W1988744333 doi "https://doi.org/10.1093/mnras/193.4.901" @default.
- W1988744333 hasPublicationYear "1980" @default.
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