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Nuclear Theory·nucl-th

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  1. A compact star rotating at 1122 Hz and the r-mode instability

    Alessandro Drago (Univ. Ferrara and INFN sez. Ferrara, Italy) Giuseppe Pagliara (Inst. Theoretische Physik, Goethe Universitaet, Frankfurt am Main, Germany and INFN Italy) · Irene Parenti (Univ. Ferrara and INFN sez. Ferrara, Italy)

    Apr 13, 2007#6*astro-phApJL21 citations

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