| A A. | |
| by | RANDICH S. , PALLAVICINI R., ANDRIEVSKY S.M., KOROTIN S.A. |
| Astron. Astrophys., 488, 943-958 (2008) | |
| Open clusters as key tracers of Galactic chemical evolution. III. Element abundances in Berkeley 20, Berkeley 29, Collinder 261, and Melotte 66. | |
| o | Table 3: <Cl* Berkeley 20 SBR NNNN> N=6 among (Nos 1201-1716), <Cl* Berkeley 29 BHT NNNN> (Nos 398, 602) added, <Cl* Melotte 66 SBR NNNN> N=7 among (Nos 1346-2218), <Cl* Collinder 261 SBR NNNN> N=7 among (Nos 2-11). |
| =E= | Catalogue in electronic form as <J/A+A/488/943/> |
====Sorry, no entry could be found==== | |