On the nature of lithium-rich giant stars Constraints from beryllium abundances

Astronomy and Astrophysics

Volumn 439, Issue 1, 2005, Pages 227-235

  Melo, C H F ^a   De Laverny, P ^b   Santos, N C ^c,d   Israelian, G ^e   Randich, S ^f   Do Nascimento Jr , J D ^g   De Medeiros, J R ^g  

^a EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c UNIVERSITY OF LISBON   (Portugal)

^d UNIVERSITÉ DE GENÈVE   (Switzerland)

^e INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^f INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^g FEDERAL UNIVERSITY OF RIO GRANDE DO NORTE   (Brazil)

Author keywords

Stars: abundances; Stars: interiors; Stars: late; Type

Indexed keywords

ASTROPHYSICS; BERYLLIUM; LITHIUM; MATHEMATICAL MODELS; MIXING; STANDARDS;

CAMERON-FOWLER PROCESS; STARS: ABUNDANCES; STARS: INTERIORS; STARS: LATE-TYPE;

ASTRONOMY;

EID: 23844532641     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041805     Document Type: Article

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