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| BCLMP 290 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.14CEST20:11:59 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1980A&AS...39...97S | 8 | 24 | A catalogue of emission regions in M 33. | SABBADIN F., RAFANELLI P. and BIANCHINI A. | |||||
2004A&A...426...11P 
|
420 | 51 | XMM-Newton survey of the Local Group galaxy M 33. | PIETSCH W., MISANOVIC Z., HABERL F., et al. | |||||
|
2006A&A...448.1247M
|
358 | 26 | An XMM-Newton survey of the Local Group galaxy M 33 - variability of the detected sources. | MISANOVIC Z., PIETSCH W., HABERL F., et al. | |||||
| 2007A&A...470..843M | 83 | 65 | The building up of the disk galaxy M33 and the evolution of the metallicity gradient. | MAGRINI L., CORBELLI E. and GALLI D. | |||||
| 2007A&A...470..865M | 92 | 101 | The metallicity gradient of M 33: chemical abundances of HII regions. | MAGRINI L., VILCHEZ J.M., MAMPASO A., et al. | |||||
|
2010A&A...512A..63M
|
15 | D | 3 | 43 | 57 | Metal production in M 33: space and time variations. | MAGRINI L., STANGHELLINI L., CORBELLI E., et al. | ||
| 2010A&A...521A..41G | 15 | D | 2 | 43 | 13 | Young stellar clusters and associations in M 33. | GROSSI M., CORBELLI E., GIOVANARDI C., et al. | ||
| 2016MNRAS.458.1866T | 97 | D | C | 6 | 38 | 62 | Carbon and oxygen abundance gradients in NGC 300 and M33 from optical recombination lines. | TORIBIO SAN CIPRIANO L., GARCIA-ROJAS J., ESTEBAN C., et al. | |
|
2020MNRAS.497..672A
|
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. | ||
|
2021ApJ...923...78S
|
17 | D | 1 | 124 | 1 | Limits to ionization-parameter mapping as a diagnostic of HII region optical depth. | SAWANT A.N., PELLEGRINI E.W., OEY M.S., et al. |
