Stellar (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>) cross sections of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Hf</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>174</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and radioactive<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Hf</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>182</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>
Christof Vockenhuber(ETH Zurich), R. Gallino(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), A. Wallner(Australian National University), W. Kutschera(University of Vienna), S. Dababneh(FZI Research Center for Information Technology), N. Winckler(Atos (France)), S. Bisterzo(University of Turin), M. Bichler(Schott (Germany)), F. Käppeler(Universitat Politècnica de Catalunya), M. Heil(Istituto Nazionale di Fisica Nucleare), I. Dillmann(GSI Helmholtz Centre for Heavy Ion Research)
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