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G30.7+1.0
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G30.7+1.0.htmlG30.71.0 ADS: search fulltext or title/keyword/abstract. Right Ascension: 18 44 00. Declination: 01 32. Size (/arcmin): 2418. Type: S? Flux density at 1 GHz (/Jy): 6. Spectral Index: 0.4. Radio: Non-thermal, highly polarised part shell? Point sources -
https://www.mrao.cam.ac.uk/projects/surveys/varies/69p.txt
https://www.mrao.cam.ac.uk/projects/surveys/varies/69p.txt30 Nov 1998: 46 00 01.9 7.3 6.3 0.14 5.9 69P9 06 01 24.24 45 58 33.3 8.1 8.6 0.16 8.1 69P10 06 ... 5 69P12 06 01 33.83 44 08 24.0 44.7 44.1 0.09 14.5 69P13 06 01 36.10 44 47 50.1 22.2 21.9 -
2nd quadrant Galactic SNRs
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.2nd.html3C434.1. Right Ascension: 21 24 50. Declination: 51 53. Size (/arcmin): 3025. ... Last updated: 24 May 2014. G106.32.7 ADS: search fulltext or title/keyword/abstract. -
G68.6-1.2
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G68.6-1.2.htmlLast updated: 24 May 2014. Dave Green / Cambridge, UK /. -
G63.7+1.1
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G63.7+1.1.htmlType: F. Flux density at 1 GHz (/Jy): 1.8. Spectral Index: 0.24. -
G320.4-1.2
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G320.4-1.2.htmlGaensler et al. 1999, MNRAS, 305, 724. ATCA at 1.4 GHz (21''24''), plus HI observations, and 5.3 GHz (10''15''). -
G85.9-0.6
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G85.9-0.6.htmlRight Ascension: 20 58 40. Declination: 44 53. Size (/arcmin): 24. -
G85.4+0.7
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G85.4+0.7.htmlRight Ascension: 20 50 40. Declination: 45 22. Size (/arcmin): 24? -
https://www.mrao.cam.ac.uk/projects/surveys/varies/68p.txt
https://www.mrao.cam.ac.uk/projects/surveys/varies/68p.txt30 Nov 1998: 35.2 68P10 06 23 56.0 42 50 42 369 408 0.09 12.5 68P11 06 24 21.0 43 22 37 186 235 0.13 8.1 68P12 ... 06 24 28.4 43 53 42 179 221 0.15 8.8 68P13 06 24 29.0 43 01 30 243 278 0.11 10.0 68P14 06 24 -
Galactic SNRs: Documentation
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.info.htmlG194.70.4 (the Origem Loop, but see below for more recent work), G287.80.5 (see below), G322.31.2 (=Kes 24) and G343.06.0 (but note that
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