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1 - 9 of 9 search results for lupus |u:www.mrao.cam.ac.uk
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  2. 4th quadrant Galactic SNRs (315

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.4thB.html
    Lupus Loop. Right Ascension: 15 10 00. Declination: 40 00. Size (/arcmin): 180?
  3. G330.0+15.0

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G330.0+15.0.html
    Lupus Loop. Right Ascension: 15 10 00. Declination: 40 00. Size (/arcmin): 180?
  4. Galactic SNRs: Documentation

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.info.html
    H153832 a large X-ray source in Lupus, near l=340, b=18 was identified as a possible SNR by Riegler, Agrawal & Gull (1980), see also Colomb, Dubner & Giacani (1984), Gahm
  5. Galactic SNRs: Other Names

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.names.html
    Galactic SNRs: Other Names. This is a (greek then numerical then alphabetical) list of the other names by which Galactic SNRs are known. Note that names in parentheses refer to part of that object only. Cassiopeia A: G111.72.1. Monoceros Nebula: G205
  6. Galactic SNRs: Summary Data

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.data.html
    Lupus Loop 330.2 1.0 16 01 06 -51 34 11 S?
  7. table-IV.dvi

    https://www.mrao.cam.ac.uk/surveys/snrs/table-IV.pdf
    10 Jan 2023: Table IV – 1 – Detailed listings. G0.0 0.0 Sgr A EastRA: 17h45m44s 1-GHz flux/Jy: 100? Size/arcmin: 3.52.5Dec: –2900′ Spectral index: 0.8? Type: S. Radio: Non-thermal shell, in complex region, interacting with molecular material to the W.
  8. table-IV.dvi

    https://www.mrao.cam.ac.uk/surveys/snrs/table-IV-l.pdf
    10 Jan 2023: Table IV – 1 – Detailed listings. G0.0 0.0 Sgr A East. RA: 17h45m44s 1-GHz flux/Jy: 100? Size/arcmin: 3.52.5Dec: –2900′ Spectral index: 0.8? Type: S. Radio: Non-thermal shell, in complex region, interacting with molecular material to the W. X
  9. tables.dvi

    https://www.mrao.cam.ac.uk/surveys/snrs/tables.pdf
    20 Feb 2023: 2022 December. – xi –. 2.3.3 X-ray/γ-ray. • H1538–32 a large X-ray source in Lupus, near l = 340, b = 18 was identified as a possible SNRby Riegler,
  10. tables.dvi

    https://www.mrao.cam.ac.uk/surveys/snrs/tables-l.pdf
    20 Feb 2023: associated radio emission. 2022 December. – xi –. 2.3.3 X-ray/γ-ray. • H1538–32 a large X-ray source in Lupus, near l = 340, b = 18 was identified as a

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