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Microquasar hadronic jets at very high-energy gamma-rays

V. Bosch-Ramon·F. A. Aharonian·J. M. Paredes
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Abstract

Microquasars (MQs) present emission over the whole spectrum, from radio wavelengths to gamma-rays. The microquasar spectral energy distribution is very complex, being a signature of the different physical processes that generate the radiation emitted by these objects. In this work, we estimate the amount of broad-band emission produced by relativistic protons, released from the jet of a MQ, interacting with high density regions of the ISM. We show that a two components source, the microquasar itself and the region of interaction between the jets and the ISM, could be unveiled by the new instruments at high-energy and very high-energy gamma-rays.

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V. Bosch-Ramon, F. A. Aharonian, J. M. Paredes. 2006-05-18. Microquasar hadronic jets at very high-energy gamma-rays. https://arxiv.org/abs/astro-ph/0605459

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