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Image for: Radioaktives Eisen - Fenster ins Innere der Sterne


Der Fingerabdruck des radioaktiven Zerfalls von Fe-60 im interstellaren Gas unserer Galaxis: In dieser Grafik sind beide Gammalinien bei ihren Sollenergien (1173 und 1332 keV) überlagert, um das schwache, mit INTEGRAL gemessene Signal sichtbar zu machen.
Der Fingerabdruck des radioaktiven Zerfalls von Fe-60 im interstellaren Gas unserer Galaxis: In dieser Grafik sind beide Gammalinien bei ihren Sollenergien (1173 und 1332 keV) überlagert, um das schwache, mit INTEGRAL gemessene Signal sichtbar zu machen.

Max-Planck-Institut für extraterrestrische Physik

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