On the nature of the AGILE galactic transient sources

TL;DR

This paper models proton-dominated jets in galactic microquasars to explain variable gamma-ray sources detected by AGILE, predicting spectral features that future Fermi observations can test.

Contribution

It introduces a comprehensive model for microquasar jets including hadronic processes, explaining AGILE's unidentified gamma-ray sources with detailed spectral predictions.

Findings

Spectral energy distributions match AGILE observations

Most power between 100 MeV and 10 GeV

Predictions testable by Fermi telescope

Abstract

The Italian gamma-ray satellite AGILE has recently reported the detection of some variable high-energy sources likely of galactic origin. These sources do not have any obvious counterpart at lower energies. We propose that these sources are produced in proton-dominated jets of galactic microquasars. We develop a model for microquasar jets that takes into account both primary leptons and protons and all relevant radiative processes, including secondary particle emission and gamma-ray attenuation due to pair creation in the jet. We obtain spectral energy distributions that correspond to what is observed by AGILE, with most of the power concentrated between 100 MeV and 10 GeV and reaching luminosities of $10^{34-35}$ erg s$^{-1}$. We make detailed spectral predictions that can be tested by the Fermi gamma-ray telescope in the immediate future. We conclude that hadronic jets in galactic accreting sources can be responsible for the variable unidentified gamma-ray sources detected by AGILE.