[DCL88] 61 , the SIMBAD biblio

[DCL88] 61 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST15:47:19


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Title First 3 Authors
1988A&AS...73..407D 179 62 H II regions in NGC 300. DEHARVENG L., CAPLAN J., LEQUEUX J., et al.
1997A&A...322...41C 22 23 A sulphur abundance study of NGC 300 by an empirical calibration method. CHRISTENSEN T., PETERSEN L. and GAMMELGAARD P.
2001A&A...371..497P viz 236 31 A catalog of OB associations in the spiral galaxy NGC 300. PIETRZYNSKI G., GIEREN W., FOUQUE P., et al.
2003A&A...397..859S 86 33 A large Wolf-Rayet population in NGC 300 uncovered by VLT-FORS2. SCHILD H., CROWTHER P.A., ABBOTT J.B., et al.
2004A&A...425..443P 86 23 Multi-frequency study of extragalactic supernova remnants and HII regions Sculptor group Sd galaxy NGC 300. PAYNE J.L., FILIPOVIC M.D., PANNUTI T.G., et al.
2005ApJ...632..227R 42 21 Extinction law variations and dust excitation in the spiral galaxy NGC 300. ROUSSEL H., GIL DE PAZ A., SEIBERT M., et al.
2009ApJ...700..309B 16       D               3 76 224 Extragalactic chemical abundances: do H II regions and young stars tell the same story? the case of the spiral galaxy NGC 300. BRESOLIN F., GIEREN W., KUDRITZKI R.-P., et al.
2012MNRAS.424.2316P viz 15       D               1 298 113 `Counterpart' method for abundance determinations in HII regions. PILYUGIN L.S., GREBEL E.K. and MATTSSON L.
2014ApJ...789...81F viz 16       D               2 82 21 Molecular cloud-scale star formation in NGC 300. FAESI C.M., LADA C.J., FORBRICH J., et al.
2016MNRAS.456.4407D viz 16       D               2 165 6 Sulphur abundance determinations in star-forming regions - I. Ionization correction factor. DORS O.L., PEREZ-MONTERO E., HAGELE G.F., et al.
2016A&A...592A..47N 40           X         1 33 4 Constraining the escape fraction of ionizing photons from HII regions within NGC 300: A concept paper. NIEDERHOFER F., HILKER M., BASTIAN N., et al.
2016MNRAS.460.1739V viz 16       D               1 615 58 BOND: Bayesian Oxygen and Nitrogen abundance Determinations in giant H II regions using strong and semistrong lines. VALE ASARI N., STASINSKA G., MORISSET C., et al.
2020MNRAS.497..672A viz 17       D               1 127 16 The Te[N II]-Te[O III] temperature relation in H II regions and the reliability of strong-line methods. ARELLANO-CORDOVA K.Z. and RODRIGUEZ M.

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