The chemical compositions of the extreme halo stars HE 0107-5240 and HE 1327-2326 inferred from three-dimensional hydrodynamical model atmospheres

Astrophysical Journal Letters

Volumn 644, Issue 2, 2006, Pages L121-L124

  Collet, R ^a   Asplund, M ^b   Trampedach, R ^b  

^a UPPSALA UNIVERSITY   (Sweden)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Convection; Galaxy: abundances; Stars: abundances; Stars: atmospheres; Stars: individual (HE 0107 5240, HE 1327 2326)

Indexed keywords

EID: 37149002344     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1086/505643     Document Type: Article

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