Cu I resonance lines in turn-off stars of NGC 6752 and NGC 6397: Effects of granulation from CO5BOLD models

Astronomy and Astrophysics

Volumn 524, Issue 4, 2010, Pages

  Bonifacio, P ^a,b,c   Caffau, E ^b,d   Ludwig, H G ^a,b,d  

^a CIFIST Marie Curie Excellence Team ^*  (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^d UNIVERSITY OF HEIDELBERG   (Germany)

Author keywords

globular clusters: general; globular clusters: individual: NGC 6397; globular clusters: individual: NGC 6752; hydrodynamics; line: formation; stars: abundances

Indexed keywords

FLUID DYNAMICS; HYDRODYNAMICS; RESONANCE; THREE DIMENSIONAL;

1-D MODELS; GIANT STARS; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: GENERAL; GLOBULAR CLUSTERS: INDIVIDUAL; HYDRODYNAMICAL MODEL; LINE: FORMATION; METALLICITIES; NGC 6752; RESONANCE LINE; STARS: ABUNDANCES;

STARS;

EID: 78649514327     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912935     Document Type: Article

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