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51 - 60 of 105 search results for katalk:PC53 24 / |u:www.mrao.cam.ac.uk where 0 match all words and 105 match some words.

  1. Results that match 1 of 2 words

  2. G18.1-0.1

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G18.1-0.1.html
    Right Ascension: 18 24 34. Declination: 13 11. Size (/arcmin): 8.

  3. G308.4-1.4

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G308.4-1.4.html
    Prinz & Becker 2012, A&A, 544, A7. ATCA at 1.4 GHz (53''64'': S=0.33 Jy) and 2.5 GHz (29''35'': S=0.24 Jy), plus Chandra and

  4. G284.3-1.8

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G284.3-1.8.html
    MSH 1053. Right Ascension: 10 18 15. Declination: 59 00. Size (/arcmin): 24?

  5. G206.9+2.3

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G206.9+2.3.html
    Odegard 1986, ApJ, 301, 813. TPT at 20.6, 25.6 and 30.9 MHz (24', 19' and 16').

  6. G309.2-0.6

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G309.2-0.6.html
    Gaensler et al. 1998, MNRAS, 299, 812. ATCA at 1.3 GHz (23''24'': S=5.20.2 Jy).

  7. G359.0-0.9

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G359.0-0.9.html
    LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''43'').

  8. G11.2-0.3

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G11.2-0.3.html
    Morsi & Reich 1987, A&AS, 71, 189. Effelsberg 100-m at 32 GHz (26.''5: S=4.040.24 Jy). ... Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.'24.'1: S=39 Jy).

  9. G31.9+0.0

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G31.9+0.0.html
    References:. Radhakrishnan et al. 1972, ApJS, 24, 49. HI absorption. ... Becker & Kundu 1976, ApJ, 204, 427. NRAO interferometer at 2.7 GHz (20''23'') and 8 GHz (9''24''), plus review of flux densities.

  10. G94.0+1.0

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G94.0+1.0.html
    3C434.1. Right Ascension: 21 24 50. Declination: 51 53. Size (/arcmin): 3025.

  11. G330.0+15.0

    https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G330.0+15.0.html
    Point sources: Central, possibly pulsating, X-ray source. References:. Milne 1971, AuJPh, 24, 757.

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