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Creators/Authors contains: "Petö, Maria_K"

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  1. ; ; ; ; ; (, Astronomische Nachrichten)
    ABSTRACT We run a three‐dimensional Galactic chemical evolution (GCE) model to follow the propagation of53Mn (exclusively produced from type Ia supernovae, SNIa),60Fe (exclusively produced from core‐collapse supernovae, CCSNe),182Hf (exclusively produced from intermediate mass stars, IMSs), and244Pu (exclusively produced from neutron star mergers, NSMs). By comparing the predictions from our three‐dimensional GCE model to recent detections of53Mn,60Fe, and244Pu on the deep‐sea floor, we draw conclusions about their propagation in the interstellar medium. 
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