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A Way Out of the Bubble Trouble?—Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth

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Zentrum für Astronomie und Astrophysik, Technische Universität Berlin, Hardenbergstraße 36, 10623 Berlin, Germany
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Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12–14, 69120 Heidelberg, Germany
*
Author to whom correspondence should be addressed.
Galaxies 2018, 6(1), 26; https://doi.org/10.3390/galaxies6010026
Received: 31 January 2018 / Revised: 20 February 2018 / Accepted: 22 February 2018 / Published: 25 February 2018
Deep-sea archives all over the world show an enhanced concentration of the radionuclide 60Fe, isolated in layers dating from about 2.2 Myr ago. Since this comparatively long-lived isotope is not naturally produced on Earth, such an enhancement can only be attributed to extraterrestrial sources, particularly one or several nearby supernovae in the recent past. It has been speculated that these supernovae might have been involved in the formation of the Local Superbubble, our Galactic habitat. Here, we summarize our efforts in giving a quantitative evidence for this scenario. Besides analytical calculations, we present results from high-resolution hydrodynamical simulations of the Local Superbubble and its presumptive neighbor Loop I in different environments, including a self-consistently evolved supernova-driven interstellar medium. For the superbubble modeling, the time sequence and locations of the generating core-collapse supernova explosions are taken into account, which are derived from the mass spectrum of the perished members of certain, carefully preselected stellar moving groups. The release and turbulent mixing of 60Fe is followed via passive scalars, where the yields of the decaying radioisotope were adjusted according to recent stellar evolution calculations. The models are able to reproduce both the timing and the intensity of the 60Fe excess observed with rather high precision. We close with a discussion of recent developments and give future perspectives. View Full-Text
Keywords: ISM: bubbles; ISM: supernova remnants; ISM: abundances; hydrodynamics; methods: numerical; methods: analytical ISM: bubbles; ISM: supernova remnants; ISM: abundances; hydrodynamics; methods: numerical; methods: analytical
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MDPI and ACS Style

Schulreich, M.M.; Breitschwerdt, D.; Feige, J.; Dettbarn, C. A Way Out of the Bubble Trouble?—Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth. Galaxies 2018, 6, 26. https://doi.org/10.3390/galaxies6010026

AMA Style

Schulreich MM, Breitschwerdt D, Feige J, Dettbarn C. A Way Out of the Bubble Trouble?—Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth. Galaxies. 2018; 6(1):26. https://doi.org/10.3390/galaxies6010026

Chicago/Turabian Style

Schulreich, Michael Mathias, Dieter Breitschwerdt, Jenny Feige, and Christian Dettbarn. 2018. "A Way Out of the Bubble Trouble?—Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth" Galaxies 6, no. 1: 26. https://doi.org/10.3390/galaxies6010026

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