Beyond the iron peak: R- and s-process elemental abundances in stars with planets

Astrophysical Journal

Volumn 682, Issue 2, 2008, Pages 1234-1247

  Bond, J C ^a   Lauretta, D S ^a   Tinney, C G ^b,c   Butler, R P ^d   Marcy, G W ^e   Jones, H R A ^f   Carter, B D ^g   O'Toole, S J ^c   Bailey, J ^h  

^a UNIVERSITY OF ARIZONA   (United States)

^b UNIVERSITY OF NEW SOUTH WALES   (Australia)

^c ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^d GEOPHYSICAL LABORATORY   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^g UNIVERSITY OF SOUTHERN QUEENSLAND   (Australia)

^h MACQUARIE UNIVERSITY   (Australia)

Author keywords

Planetary systems; Stars: abundances; Stars: chemically peculiar

Indexed keywords

EID: 53549133394     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/589236     Document Type: Article

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