The effect of heavy element opacity on pre-main sequence Li depletion

Astronomy and Astrophysics

Volumn 454, Issue 1, 2006, Pages 311-319

  Sestito, P ^a,b   Degl'Innocenti, S ^c,d   Prada Moroni, P G ^c,d   Randich, S ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c UNIVERSITY OF PISA   (Italy)

^d INFN SEZIONE DI PISA   (Italy)

Author keywords

Stars: abundances; Stars: evolution; Stars: interiors

Indexed keywords

ASTROPHYSICS; COMPOSITION; OPACITY; SOLAR SYSTEM; SPACE RESEARCH; THERMAL EFFECTS;

METALLICITY; STARS: ABUNDANCES; STARS: EVOLUTION; STARS: INTERIORS;

LITHIUM COMPOUNDS;

EID: 33746349536     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054605     Document Type: Article

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