LHA 120-N 193C , the SIMBAD biblio

LHA 120-N 193C , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST13:06:36

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1956ApJS....2..315H 911 846 Catalogues of H-alpha emission stars and nebulae in the Magellanic Clouds. HENIZE K.G.
1976MmRAS..81...89D viz 603 555 The nebular complexes of the Large and Small Magellanic Clouds. DAVIES R.D., ELLIOTT K.H. and MEABURN J.
1983A&AS...54..459G 106 50 Observations of giant bubbles in the Large Magellanic Cloud. GEORGELIN Y.M., GEORGELIN Y.P., LAVAL A., et al.
1987RMxAA..14..178P 17 2 Spectrophotometric observations of very low ionization HII regions in the LMC. PENA M., RUIZ M.T. and RUBIO M.
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..125..419L viz 799 45 Obscured AGB stars in the Magellanic Clouds. I. IRAS candidates. LOUP C., ZIJLSTRA A.A., WATERS L.B.F.M., et al.
1999AJ....117..238B viz 6184 135 A revised and extended catalog of Magellanic system clusters, associations, and emission nebulae. II. The Large Magellanic Cloud. BICA E.L.D., SCHMITT H.R., DUTRA C.M., et al.
2008MNRAS.389..678B viz 15       D               2 9123 164 A general catalogue of extended objects in the Magellanic System. BICA E., BONATTO C., DUTRA C.M., et al.
2012ApJ...755...40P viz 15       D               1 636 137 The optical depth of H II regions in the Magellanic Clouds. PELLEGRINI E.W., OEY M.S., WINKLER P.F., et al.
2017ApJ...844...63O 40           X         1 440 ~ Dust emission at 8 and 24 µm as diagnostics of H II region radiative transfer. OEY M.S., LOPEZ-HERNANDEZ J., KELLAR J.A., et al.
2018MNRAS.480.2743F 16       D               2 23 6 A multifrequency radio continuum study of the Magellanic Clouds - I. Overall structure and star formation rates. FOR B.-Q., STAVELEY-SMITH L., HURLEY-WALKER N., et al.

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