Improved laboratory transition probabilities for ce ii, application to the cerium abundances of the sun and five r-process-rich, metal-poor stars, and rare earth lab data summary

Astrophysical Journal, Supplement Series

Volumn 182, Issue 1, 2009, Pages 51-79

  Lawler, J E ^a   Sneden, C ^b,c   Cowan, J J ^d   Ivans, I I ^e,f   Den Hartog, E A ^a  

^a University of Wisconsin Madison   (United States)

^b The University of Texas at Austin   (United States)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^d UNIVERSITY OF OKLAHOMA   (United States)

^e CARNEGIE OBSERVATORIES   (United States)

^f PRINCETON UNIVERSITY OBSERVATORY   (United States)

Author keywords

Atomic data; Galaxy: evolution; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: individual (BD+17?3248, CS 22892052, CS 31082001, HD 115444, HD 221170); Stars: Population II; Sun: abundances

Indexed keywords

EID: 67650973672     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1088/0067-0049/182/1/51     Document Type: Article

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