Can We Draw Conclusions on Supernova Shock Wave Propagation Using Short-Lived Radioactive Isotopes?

Wehmeyer, Benjamin, López, Andrés Yagüe, Côté, Benoit, Peto, Mária K., Kobayashi, Chiaki and Lugaro, Maria (2025) Can We Draw Conclusions on Supernova Shock Wave Propagation Using Short-Lived Radioactive Isotopes? Astronomische Nachrichten: e70002. pp. 1-6. ISSN 0004-6337

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We run a three-dimensional Galactic chemical evolution (GCE) model to follow the propagation of 53Mn (exclusively produced from type Ia supernovae, SNIa), 60Fe (exclusively produced from core-collapse supernovae, CCSNe), 182Hf (exclusively produced from intermediate mass stars, IMSs), and 244Pu (exclusively produced from neutron star mergers, NSMs). By comparing the pre- dictions from our three-dimensional GCE model to recent detections of 53Mn, 60Fe, and 244Pu on the deep-sea floor, we draw conclusions about their propagation in the interstellar medium.

Item Type	Article
Additional information	© 2025 The Author(s). Astronomische Nachrichten published by Wiley-VCH GmbH. This is an open access article distributed under the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
Keywords	astrochemistry, galactic abundances, interstellar medium
Date Deposited	30 May 2025 14:10
Last Modified	31 May 2025 00:48