Context. It has been proposed that the origin of the very high-energy photons emitted from high-mass X-ray binaries with jet-like features, so-called microquasars (MQs), is related to hadronic interactions between relativistic protons in the jet and cold protons of the stellar wind. Leptonic secondary emission should be calculated in a complete hadronic model that include the effects of pairs from charged pion decays inside the jets and the emission from pairs generated by gamma-ray absorption in the photosphere of the system. Aims. We aim at predicting the broadband spectrum from a general hadronic microquasar model, taking into account the emission from secondaries created by charged pion decay inside the jet. Methods. The particle energy...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...
We present a one–zone jet model that fits the data from simultaneous broadband radio-to-X-rays obser...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...
Context.It has been proposed that the origin of the very high-energy photons emitted from high-mass ...
Observational and theoretical studies point to microquasars (MQs) as possible counterparts of a sign...
We present a model to estimate the synchrotron radio emission generated in microquasar (MQ) jets due...
We present a general self-consistent lepto/hadronic jet model for the non-thermal electromagnetic em...
We present a general self-consistent lepto/hadronic jet model for the non-thermal electromagnetic em...
Unlike high-mass gamma-ray binaries, low-mass microquasars lack external sources of radiation and ma...
In this work we present a new jet model for the non-thermal broadband emission of low-mass microquas...
he Galactic high-mass X-ray binary and jet source (microquasar) LSI +61 303 has recently been detect...
Observational and theoretical studies point to microquasars (MQs) as possible counterparts of a sign...
Microquasars are X-ray binary systems that present relativistic radio jets.These systems consist on ...
Microquasars are sources of very high-energy gamma-rays and, very probably, high-energy gamma-ray em...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...
We present a one–zone jet model that fits the data from simultaneous broadband radio-to-X-rays obser...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...
Context.It has been proposed that the origin of the very high-energy photons emitted from high-mass ...
Observational and theoretical studies point to microquasars (MQs) as possible counterparts of a sign...
We present a model to estimate the synchrotron radio emission generated in microquasar (MQ) jets due...
We present a general self-consistent lepto/hadronic jet model for the non-thermal electromagnetic em...
We present a general self-consistent lepto/hadronic jet model for the non-thermal electromagnetic em...
Unlike high-mass gamma-ray binaries, low-mass microquasars lack external sources of radiation and ma...
In this work we present a new jet model for the non-thermal broadband emission of low-mass microquas...
he Galactic high-mass X-ray binary and jet source (microquasar) LSI +61 303 has recently been detect...
Observational and theoretical studies point to microquasars (MQs) as possible counterparts of a sign...
Microquasars are X-ray binary systems that present relativistic radio jets.These systems consist on ...
Microquasars are sources of very high-energy gamma-rays and, very probably, high-energy gamma-ray em...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...
We present a one–zone jet model that fits the data from simultaneous broadband radio-to-X-rays obser...
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observe...