Sulfur in the globular clusters 47 Tucanae and NGC 6752

Astronomy and Astrophysics

Volumn 503, Issue 1, 2009, Pages 121-127

  Sbordone, L ^a,b   Limongi, M ^c   Chieffi, A ^d   Caffau, E ^b   Ludwig, H G ^a,b   Bonifacio, P ^a,b,e  

^a CIFIST Marie Curie Excellence Team   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^d INAF IASF ROMA   (Italy)

^e INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

Author keywords

Galaxy: globular clusters: individual: NGC 104; Galaxy: globular clusters: individual: NGC 6752; Stars: abundances

Indexed keywords

ATOMIC DIFFUSIONS; GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: NGC 6752; GALAXY:GLOBULAR CLUSTERS; GIANT STARS; GLOBULAR CLUSTERS; HIGH-RESOLUTION SPECTRA; HYDRODYNAMIC MODEL; IN-FIELD; LIGHT ELEMENTS; METALLICITIES; NGC 6752; PLANE-PARALLEL MODEL; SPECTRUM SYNTHESIS; STARS: ABUNDANCES; STATISTICAL SIGNIFICANCE;

CHEMICAL ELEMENTS; GALAXIES; SODIUM; SULFUR;

STARS;

EID: 77957897275     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811513     Document Type: Article

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