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Nonthermal emission from high-mass microquasar jets affected by orbital motion
Edgar Molina, Valentí Bosch-Ramon
The stellar wind in high-mass microquasars should interact with the jet. This interaction, coupled with orbital motion, is expected to make the jet follow a helical, nonballistic t…
The influence of the optical star on the jets of high-mass microquasars
Edgar Molina, Valentí Bosch-Ramon
Microquasars are binary systems consisting of a compact object and a star that present relativistic jets. When the companion is a high-mass star, significant interaction between th…
The role of AGN jets in the reionization epoch
V. Bosch-Ramon
The reionization of the Universe ends the dark ages that started after the recombination era. In the case of H, reionization finishes around . Faint star-forming galaxies…
Constraining very-high-energy and optical emission from FRB 121102 with the MAGIC telescopes
MAGIC Collaboration, V. A. Acciari, S. Ansoldi +155
Fast radio bursts (FRBs) are bright flashes observed typically at GHz frequencies with millisecond duration, whose origin is likely extragalactic. Their nature remains mysterious,…
Inverse Compton Emission from Relativistic Jets in Binary Systems
D. Khangulyan, V. Bosch-Ramon, Y. Uchiyama
The gamma-ray emission detected from several microquasars can be produced by relativistic electrons emitting through inverse Compton scattering. In particular, the GeV emission det…
Multi-zone non-thermal radiative model for stellar bowshocks
S. del Palacio, V. Bosch-Ramon, A. L. Müller +1
Context: Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43…