NGC 5450 , the SIMBAD biblio

NGC 5450 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST21:06:51


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Title First 3 Authors
1987ApJS...63..809S 486 53 The Case low-dispersion northern sky survey. IV. Galaxies in the Bootes void region. SANDULEAK N. and PESCH P.
1990ApJS...73..661H viz 1273 32 The HII regions of M 101. I. An atlas of 1264 emission regions. HODGE P.W., GURWELL M., GOLDADER J.D., et al.
1996ApJ...456..504K 1 49 169 The composition gradient in M101 revisited. I. H II region spectra and excitation properties. KENNICUTT R.C.Jr and GARNETT D.R.
2000MNRAS.312..130D 141 87 An empirical calibration of nebular abundances based on the sulphur emission lines. DIAZ A.I. and PEREZ-MONTERO E.
2000MNRAS.317...55S viz 14       D               1 16418 457 The PSCz catalogue. SAUNDERS W., SUTHERLAND W.J., MADDOX S.J., et al.
2001ARep...45..581B viz 15       D               1 1482 6 Properties of quasar-galaxy associations and gravitational mesolensing by halo objects. BUKHMASTOVA Y.L.
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2003ApJ...591..801K 3 38 380 The composition gradient in M101 revisited. II. Electron temperatures and implications for the nebular abundance scale. KENNICUTT R.C.Jr, BRESOLIN F. and GARNETT D.R.
2006A&A...449..193P 147 22 An empirical calibration of sulphur abundance in ionised gaseous nebulae. PEREZ-MONTERO E., DIAZ A.I., VILCHEZ J.M., et al.
2010ApJS..188...46K 38           X         1 24 32 The Chandra M101 megasecond: diffuse emission. KUNTZ K.D. and SNOWDEN S.L.
2013ApJ...766...17L 39           X         1 55 29 Testing for azimuthal abundance gradients in M101. LI Y., BRESOLIN F. and KENNICUTT R.C.Jr
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.
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.
2016ApJ...830....4C viz 136       D     X         4 118 106 CHAOS III: gas-phase abundances in NGC 5457. CROXALL K.V., POGGE R.W., BERG D.A., et al.
2017MNRAS.467..102C 244           X   F     5 15 ~ Red supergiant stars in NGC 4449, NGC 5055 (M63) and NGC 5457 (M101). CHUN S.-H., SOHN Y.-J., ASPLUND M., et al.
2018AJ....155...17C viz 16       D               1 803 ~ Infrared photometric study of Wolf-Rayet galaxies. CHEN P.S., YANG X.H., LIU J.Y., et al.
2020ApJ...893...96B viz 17       D               1 204 65 CHAOS IV: gas-phase abundance trends from the first four CHAOS galaxies. BERG D.A., POGGE R.W., SKILLMAN E.D., et al.
2020MNRAS.497..672A viz 17       D               3 127 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.
2021ApJ...912..103C 88             C       1 7 11 Benchmarking dust emission models in M101. CHASTENET J., SANDSTROM K., CHIANG I.-D., et al.

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