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| HGGK 972 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST23:24:16 |
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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 
|
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. | |||||
| 1996AJ....112.1009B | 1 | 8 | 27 | An HST study of OB associations and star clusters in M101. | BRESOLIN F., KENNICUTT R.C.Jr and STETSON P.B. | ||||
| 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. | |||||
| 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. | ||||
| 2007ApJ...656..186B | 3 | 18 | 125 | The oxygen abundance in the inner H II regions of M 101: implications for the calibration of strong-line metallicity indicators. | BRESOLIN F. | ||||
| 2013ApJ...766...17L | 172 | D | X C | 4 | 55 | 29 | Testing for azimuthal abundance gradients in M101. | LI Y., BRESOLIN F. and KENNICUTT R.C.Jr | |
|
2016MNRAS.460.1739V
|
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
|
16 | D | 2 | 118 | 106 | CHAOS III: gas-phase abundances in NGC 5457. | CROXALL K.V., POGGE R.W., BERG D.A., et al. | ||
|
2020ApJ...893...96B
|
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. |
