Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble - I. 60Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous interstellar medium

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Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble - I. 60Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous interstellar medium | Astronomy & Astrophysics (A&A)

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Volume 604 (August 2017)

A&A, 604 (2017) A81

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Fig. 7

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Local interstellar fluence of ⁶⁰Fe atoms due to each individual SN in the LB volume (see legends) as a function of time before present in models A (upper panel) and B (lower panel). The inlays are zoom-ins on the last group of peaks, respectively.

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