Improved laboratory transition probabilities for Hf II and hafnium abundances in the sun and 10 metal-poor stars

Astrophysical Journal, Supplement Series

Volumn 169, Issue 1, 2007, Pages 120-136

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

^a University of Wisconsin Madison   (United States)

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

^c UNIVERSITY OF OKLAHOMA   (United States)

^d CARNEGIE OBSERVATORIES   (United States)

^e PRINCETON UNIVERSITY OBSERVATORY   (United States)

Author keywords

Atomic data; Galaxy: evolution; Nuclear reactions, nucleosynthesis, abundances; Stars: individual (HD 74462, HD 115444, HD 122956, HD 165195, HD 175305, HD 186478, HD 221170, BD +17 3248, CS 22892 052, CS 31082 001); Sun: abundances

Indexed keywords

EID: 34047199981     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/510368     Document Type: Article

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