Determination of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>141</mml:mn></mml:msup></mml:math>Pr(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mspace width="-0.16em"/><mml:mi>n</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>144</mml:mn></mml:msup></mml:math>Pm cross sections at energies of relevance for the astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi></mml:math>process using the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>γ</mml:mi><mml:mi>γ</mml:mi></mml:mrow></mml:math>coincidence method
A. Sauerwein(University of Cologne), A. Zilges(University of Cologne), Detlef Rogalla(University Hospitals of the Ruhr-University of Bochum), H. Dombrowski(Physikalisch-Technische Bundesanstalt), J. Endres(University of Cologne), L. Netterdon(University of Cologne), J. Hasper(University of Cologne), Harry Becker(Ruhr University Bochum), U. Giesen(Physikalisch-Technische Bundesanstalt), Andreas Hennig(University of Cologne), T. Rauscher(University of Hertfordshire), K. O. Zell(University of Cologne), M. Elvers(University of Cologne)
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