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

Astrophysical Journal, Supplement Series

Volumn 167, Issue 2, 2006, Pages 292-314

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

^a UNIVERSITY OF WISCONSIN MADISON   (United States)

^b Section of Molecular Genetics and Microbiology   (United States)

^c UNIVERSITY OF OKLAHOMA   (United States)

Author keywords

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

Indexed keywords

EID: 33845990613     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/508262     Document Type: Article

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