Details on Acronym: Cl* Berkeley 32 SBR | |
| Cl* Berkeley 32 SBR | (Sestito+Bragaglia+Randich+) |
| Write: | <<Cl* Berkeley 32 SBR NNN>> |
| N: | 10 |
| Object: | *inCl |
| Ref: | =2006A&A...458..121S |
| by | SESTITO P. , BRAGAGLIA A., RANDICH S., CARRETTA E., PRISINZANO L., TOSI M. |
| Astron. Astrophys., 458, 121-134 (2006) | |
| Old open clusters as key tracers of Galactic chemical evolution. I. Fe abundances in NGC 2660, NGC 3960, and Berkeley 32. | |
| o | Table 3, col(1): <Cl* NGC 3960 SBR cN> (Nos c1 to c9). Table 5, col(1): < Cl* Berkeley 32 SBR NNN> N=10 among (Nos 17-941). |