Stellar neutron capture on promethium: Implications for the s-process neutron density

Astrophysical Journal

Volumn 582, Issue 2 I, 2003, Pages 1251-1262

  Reifarth, R ^a   Arlandini, C ^a   Heil, M ^a   Kappeler F ^a   Sedyshev, P V ^b   Mengoni, A ^c   Herman, M ^d   Rauscher, T ^e   Gallino, R ^f   Travaglio, C ^g,h  

^a KARLSRUHE INSTITUTE OF TECHNOLOGY   (Germany)

^b JOINT INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

^c Ente Naz Nuove Tecn Ener/A   (Italy)

^d INTERNATIONAL ATOMIC ENERGY AGENCY   (Austria)

^e UNIVERSITY OF BASEL   (Switzerland)

^f UNIVERSITY OF TURIN   (Italy)

^g MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^h OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

Author keywords

Methods: laboratory; Nuclear reactions, nucleosynthesis, abundances; Stars: late type

Indexed keywords

EID: 0242574933     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344718     Document Type: Article

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