HGGK 128 , the SIMBAD biblio

HGGK 128 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:37:20

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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
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 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.
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.
2008ApJ...682..336G 19       D               1 24 196 The behavior of the aromatic features in M101 H II regions: evidence for dust processing. GORDON K.D., ENGELBRACHT C.W., RIEKE G.H., et al.
2009MNRAS.398..485P 82 16 On the electron temperatures in high-metallicity HII regions. PILYUGIN L.S., MATTSSON L., VILCHEZ J.M., 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.
2013ApJ...766...17L 445     A     X C       11 55 29 Testing for azimuthal abundance gradients in M101. LI Y., BRESOLIN F. and KENNICUTT R.C.Jr
2016MNRAS.456.4407D viz 16       D               2 164 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 16       D               3 118 106 CHAOS III: gas-phase abundances in NGC 5457. CROXALL K.V., POGGE R.W., BERG D.A., et al.
2020ApJ...893...96B viz 16       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.
2020ApJ...894..138S 16       D               1 17 ~ CHAOS V: recombination line carbon abundances in M 101. SKILLMAN E.D., BERG D.A., POGGE R.W., et al.
2020MNRAS.497..672A viz 16       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.
2024ApJ...971...87B 18       D               5 18 ~ CHAOS. VIII. Far-ultraviolet Spectra of M101 and the Impact of Wolf-Rayet Stars. BERG D.A., SKILLMAN E.D., CHISHOLM J., et al.

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