First stars IV. CS 29497-030: Evidence for operation of the s-process at very low metallicity

Astronomy and Astrophysics

Volumn 413, Issue 3, 2004, Pages 1073-1085

  Sivarani, T ^a   Bonifacio, P ^a   Molaro, P ^a   Cayrel, R ^b   Spite, M ^b   Spite, F ^b   Plez, B ^c   Andersen, J ^d   Barbuy, B ^e   Beers, T C ^f   Depagne, E ^g   Hill, V ^b   Francois P ^b   Nordstrom B ^d,h   Primas, F ⁱ  

^a INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIV MONTPELLIER   (France)

^d NBIfAFG ^*  (Denmark)

^e UNIVERSITY OF SÃO PAULO   (Brazil)

^f MICHIGAN STATE UNIVERSITY   (United States)

^g EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^h LUND UNIVERSITY   (Sweden)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxy: abundances; Galaxy: halo; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: binary: spectroscopic; Stars: individual: CS29497 030

Indexed keywords

ABSORPTION; CARBON; GALAXIES; LEAD; NEUTRONS; NUCLEAR PHYSICS; SPECTROSCOPIC ANALYSIS; THERMOANALYSIS;

NUCLEOSYNTHESIS; STARS; THERMALLY PULSING (TP);

ASTROPHYSICS;

EID: 10744222770     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031590     Document Type: Article

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