出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：If the jets ofmicroquasars carry a significant power in the formof relativistic hadrons, then gamma
rays and neutrinos can be produced by interactions with matter and photon fields either external
or internal to the jet. In this paper I present some recent results of calculations of the interaction
of hadronic jets with 1) matter of the jet itself, 2) photon fields generated by synchrotron radiation
of both protons and electrons, and 3) matter external to the jet (e.g. a clumped wind). I briefly
discuss neutrino production in these scenarios and the prospects of detection with new gamma-ray
instruments. Finally, I make a few comments on the controversy about the nature of LS I +61 303.
