Heavy element abundances in cool dwarf stars: An implication for the evolution of the Galaxy

Astronomy and Astrophysics

Volumn 376, Issue 1, 2001, Pages 232-247

  Mashonkina, L ^a,b,c   Gehren, T ^b  

^a KAZAN FEDERAL UNIVERSITY   (Russian Federation)

^b UNIVERSITY OF MUNICH   (Germany)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Galaxy: evolution; Line: formation; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: late type

Indexed keywords

EID: 0035443417     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010965     Document Type: Article

References (69)