| |
Barbuy, B. |
| Volume |
Paper Title |
Page Number |
Authors |
| 9 |
CNO in red giants |
328 |
Barbuy, B. |
| 26 |
Strong ^13CN Lines in Barium Stars |
582 |
Barbuy, B.; Jorissen, A.; Rossi, S. C. F. |
| 114 |
Chemical Composition of Old Stars |
51 |
Barbuy, B. |
| 245 |
First Measurement of the Uranium/Thorium Ratio in a Very Old Star: Implications for the Age of the Galaxy |
244 |
Cayrel, R.; Spite, M.; Spite, F.; Hill, V.; Primas, F.; François, P.; Beers, T. C.; Plez, B.; Barbuy, B.; Andersen, J.; Nordström, B.; Molaro, P.; Bonifacio, P. |
| 265 |
B,V and V,I Color-Magnitude Diagrams of ω Centauri Compared to Templates |
325 |
Barbuy, B.; Ortolani, S. |
| 296 |
VLT-UVES Spectroscopy of the Subgiant I-24 of the Bulge Globular Cluster NGC 6528 in Baade's Window |
358 |
Barbuy, B.; Dutra, C.; Hill, V.; Ortolani, S.; Momany, Y.; Bica, E.; Renzini, A.; Zoccali, M.; Pasquini, L.; Minniti, D.; Rich, R. M. |
| 304 |
Oxygen Abundances in Metal-Poor stars |
88 |
Barbuy, B.; Melendez, J. |
| 491 |
Metallicities and Alpha-to-Iron Ratios in Globular Cluster Stars on a
Homogeneous Scale: Search for Multiple Populations |
134 |
Dias, B.; Saviane, I.; Barbuy, B.; Held, E.; Da Costa, G.; Ortolani, S.; Vasquez, S. |
| 491 |
Self-Consistent Physical Parameters for 5 Intermediate-Age SMC Stellar Clusters from CMD Modeling |
338 |
Dias, B.; Kerber, L.; Barbuy, B.; Santiago, B.; Ortolani, S.; Balbinot, E. |
|
|
