Beryllium abundances and star formation in the halo and in the thick disk

Astronomy and Astrophysics

Volumn 499, Issue 1, 2009, Pages 103-119

  Smiljanic, R ^a,b   Pasquini, L ^b   Bonifacio, P ^c,d   Galli, D ^e   Gratton, R G ^f   Randich, S ^e   Wolff, B ^b  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

Author keywords

Galaxy: disk; Galaxy: halo; Stars: abundances; Stars: late type

Indexed keywords

ANTICORRELATION; ATMOSPHERIC PARAMETERS; EVOLUTIONARY MODELS; GALAXY: DISK; GALAXY: HALO; HALO STARS; HIGH RESOLUTION; LOCAL CONDITIONS; METALLICITY; ORBITAL PARAMETERS; SIGNAL TO NOISE; SPECTRUM SYNTHESIS; STAR FORMATION RATES; STAR FORMATIONS; STARS: ABUNDANCES; STARS: LATE-TYPE; STATISTICAL DETECTION; THICK DISK; TWO-COMPONENT;

BERYLLIUM; COSMOLOGY; DISKS (STRUCTURAL COMPONENTS); GALAXIES; GRAPHIC METHODS; IONIZING RADIATION; KINEMATICS; MEASUREMENT ERRORS; ORBITAL LABORATORIES;

STARS;

EID: 66349135666     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810592     Document Type: Article

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