Abstract
The natural sources of neutrinos and the energy of neutrinos derived from these sources are described. The present knowledge of the neutrino properties which most affect the astrophysics of neutrinos (such as the number of families and the neutrino mass, magnetic moment, and lifetime) is reviewed. The present neutrino telescopes and the telescopes planned for the 1990s are described, together with their threshold, mass, area, and angular resolution properties. Special attention is given to the supernova neutrino detectors. 8 refs.
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