TY  - CHAP 
AU  - Beckman, John E.
AU  - Casuso, Emilio
AU  - Zurita Muñoz, Almudena
AU  - Relaño Pastor, Mónica
PY  - 2004
SN  - 1-4020-2861-X
UR  - http://hdl.handle.net/10481/29036
AB  - In the first part of this article we show how observations of the chemical evolution of the Galaxy: G- and K-dwarf numbers as functions of metallicity, and abundances of the light elements, D, Li, Be and B, in both stars and the interstellar medium...
LA  - eng
PB  - Springer
KW  - Galaxy
KW  - Evolution
KW  - Accretion
KW  - ISM
KW  - Kinematics
KW  - Star formation
TI  - Gas flows, star formation and galaxy evolution
ER  -