  Evidence for a local 'Single Source' of cosmic rays is amassing by way of the
recent precise measurements of various cosmic ray energy spectra from the
AMS-02 instrument. To observations of individual cosmic ray nuclei, electrons,
positrons and antiprotons must now be added the determination of the
boron-to-carbon ratio and the energy spectrum of lithium to 2000 GV with high
precision. Our analysis leads us to claim that, with certain assumptions about
propagation in the Galaxy, the results confirm our arguments regarding the
presence of a local single source, perhaps, a supernova remnant (SNR). An
attempt is made to determine some of the properties of this SNR and its
progenitor star.

High Energy Astrophysical Phenomena