PMN J0533-6845 , the SIMBAD biblio

PMN J0533-6845 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:37:31


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Title First 3 Authors
1972AuJPh..25..613M 8 21 The radio continuum of the Large Magellanic Cloud. III. The sources at 11 cm wavelength. McGEE R.X., BROOKS J.W. and BATCHELOR R.A.
1994ApJS...91..111W viz 4374 324 The Parkes-MIT-NRAO (PMN) Surveys: II. Source catalog for the Southern Survey (-87deg.5 < delta < -37deg). WRIGHT A.E., GRIFFITH M.R., BURKE B.F., et al.
1995A&AS..111..311F viz 713 51 A radio continuum study of the Magellanic Clouds. IV. Catalogues of radio sources in the Large Magellanic Cloud at 1.40, 2.45, 4.75, 4.85 and 8.55 GHz. FILIPOVIC M.D., HAYNES R.F., WHITE G.L., et al.
1997A&AS..126..325M viz 126 24 A catalogue of compact radio sources in and behind the Large Magellanic Cloud. MARX M., DICKEY J.M. and MEBOLD U.
1998A&AS..130..421F viz 716 83 A radio continuum study of the Magellanic Clouds. VII. Discrete radio sources in the Magellanic Clouds. FILIPOVIC M.D., HAYNES R.F., WHITE G.L., et al.
1998A&AS..130..441F 174 13 A radio continuum study of the Magellanic Clouds. VIII. Discrete sources common to radio and infrared surveys of the Magellanic Clouds. FILIPOVIC M.D., JONES P.A., WHITE G.L., et al.
2000A&A...354..787M 42 31 A study of the cool gas in the Large Magellanic Cloud. I. Properties of the cool atomic phase - a third HI absorption survey. MARX-ZIMMER M., HERBSTMEIER U., DICKEY J.M., et al.
2010A&A...511A..53V viz 15       D               1 107473 39 The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. VOLLMER B., GASSMANN B., DERRIERE S., et al.
2012ApJ...759...25M viz 38           X         1 23 30 Magnetic field structure of the Large Magellanic Cloud from Faraday rotation measures of diffuse polarized emission. MAO S.A., McCLURE-GRIFFITHS N.M., GAENSLER B.M., et al.
2021A&A...655A..17S viz 17       D               1 338578 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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