Improved laboratory transition probabilities for Sm II and application to the Samarium abundances of the sun and three r-process-rich, metal-poor stars

Astrophysical Journal, Supplement Series

Volumn 162, Issue 1, 2006, Pages 227-260

  Lawler, J E ^a   Den Hartog, E A ^a   Sneden, C ^b   Cowan, J J ^c  

^a University of Wisconsin Madison   (United States)

^b UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^c UNIVERSITY OF OKLAHOMA   (United States)

Author keywords

Atomic data; Stars: abundances; Stars: Population II; Sun: abundances

Indexed keywords

EID: 33644547014     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/498213     Document Type: Article

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