Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble - II. Advanced modelling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernova activity in the solar neighbourhood

Open Access

Fig. 1

IMFs of those Sco-Cen populations in which SN explosions should have already occurred (curves). Each mass bin of the respectively derived histograms (colours correspond) contains a single progenitor star.

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