Details on Acronym: Cl* NGC 3960 SBR | |
Cl* NGC 3960 SBR | (Sestito+Bragaglia+Randich+) |
Write: | <<Cl* NGC 3960 SBR cN>> |
N: | 9 |
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). |