Authors:
Romano, D
Matteucci, F
Ventura, P
D'Antona, F
Citation: D. Romano et al., The stellar origin of Li-7 - Do AGB stars contribute a substantial fraction of the local Galactic lithium abundance?, ASTRON ASTR, 374(2), 2001, pp. 646-655
Citation: F. Matteucci et S. Recchi, On the typical timescale for the chemical enrichment from Type Ia supernovae in galaxies, ASTROPHYS J, 558(1), 2001, pp. 351-358
Authors:
Colafrancesco, S
Mullis, CR
Wolter, A
Gioia, IM
Maccacaro, T
Antonelli, A
Fiore, F
Kaastra, J
Mewe, R
Rephaeli, Y
Fusco-Femiano, R
Antonuccio-Delogu, V
Matteucci, F
Mazzotta, P
Citation: S. Colafrancesco et al., An X-ray and optical study of the cluster A33, ASTR AST SS, 144(2), 2000, pp. 187-194
Authors:
Romano, D
Matteucci, F
Salucci, P
Chiappini, C
Citation: D. Romano et al., The mass surface density in the local disk and the chemical evolution of the Galaxy, ASTROPHYS J, 539(1), 2000, pp. 235-240
Authors:
Gratton, RG
Carretta, E
Matteucci, F
Sneden, C
Citation: Rg. Gratton et al., Abundances of light elements in metal-poor stars IV. [Fe/O] and [Fe/Mg] ratios and the history of star formation in the solar neighborhood, ASTRON ASTR, 358(2), 2000, pp. 671-681
Citation: A. Martinelli et F. Matteucci, A possible solution of the G-dwarf problem in the frame-work of closed models with a time-dependent IMF, ASTRON ASTR, 353(1), 2000, pp. 269-275
Citation: R. Jimenez et al., On the origin of damped Ly alpha systems: A case for low surface brightness galaxies?, ASTROPHYS J, 514(2), 1999, pp. L83-L86