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CCM 54 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST11:21:33 |
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 |
---|---|---|---|---|---|---|---|---|---|
1996A&A...309..446P | 491 | 25 | The spiral structure of M 51 from Hα and 2000A UV images. A new tracer of density waves. | PETIT H., HUA C.T., BERSIER D., et al. | |||||
2004ApJ...615..228B | 1 | 37 | 197 | Abundances of metal-rich H II regions in M51. | BRESOLIN F., GARNETT D.R. and KENNICUTT R.C.Jr | ||||
2005A&A...436L...1P | 16 | 18 | On the relationship between auroral and nebular oxygen line intensities in spectra of HII regions. | PILYUGIN L.S. | |||||
2005ApJ...631..231P | 6 | 20 | 406 | Oxygen abundance determination in H II regions: the strong line intensities-abundance calibration revisited. | PILYUGIN L.S. and THUAN T.X. | ||||
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. | |||||
2006MNRAS.367.1139P | 2 | 13 | 52 | Oxygen abundances in the most oxygen-rich spiral galaxies. | PILYUGIN L.S., THUAN T.X. and VILCHEZ J.M. | ||||
2009MNRAS.398..485P | 15 | D | 1 | 82 | 16 | On the electron temperatures in high-metallicity HII regions. | PILYUGIN L.S., MATTSSON L., VILCHEZ J.M., et al. | ||
2010ApJS..190..233M | 15 | D | 1 | 353 | 439 | Optical spectroscopy and nebular oxygen abundances of the Spitzer/SINGS galaxies. | MOUSTAKAS J., KENNICUTT R.C.Jr, TREMONTI C.A., et al. | ||
2012MNRAS.424.2316P | 15 | D | 2 | 298 | 113 | `Counterpart' method for abundance determinations in HII regions. | PILYUGIN L.S., GREBEL E.K. and MATTSSON L. | ||
2015ApJ...808...42C | 16 | D | 2 | 70 | 76 | CHAOS II. Gas-phase abundances in NGC 5194. | CROXALL K.V., POGGE R.W., BERG D.A., et al. | ||
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. | ||
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. |