Stars within 10 parsec from the Sun and their neutrino fluxes at Earth

摘要

The shapes of neutrino spectra and fluxes from representative stars in the solar neighborhood up to 10 parsec are calculated. The individual contribution of the most important, specific stellar objects (the α-Centauri system, Sirius A, Procyon, Vega, Fomalhaut and Altair) are determined and investigated by detailed stellar modeling. The possibility for a potential detection is discussed.