activity
20062025
most citedSensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

135 citations · 1.2k across the 53 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.HE2010★ 1 cited

Radiation from matter entrainment in astrophysical jets: the AGN case

Anabella T. Araudo, Valenti Bosch-Ramon, Gustavo E. Romero

Jets are found in a variety of astrophysical sources, from young stellar objects to active galactic nuclei. In all the cases the jet propagates with a supersonic velocity through t…

astro-ph.HE2010

Non-thermal radiation from a runaway massive star

Gustavo E. Romero, Paula Benaglia, Cintia S. Peri +2

We present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under…

astro-ph.HE2010★ 2 cited

Non-thermal radiation associated with astrophysical shock waves

Anabella T. Araudo

The main goal of this thesis is to study the physical processes that can produce non-thermal emission at high energies in astrophysical objects capable to accelerate particles up t…

astro-ph.SR2010★ 81 cited

Detection of nonthermal emission from the bow shock of a massive runaway star

Paula Benaglia, Gustavo E. Romero, Josep Marti +2

The environs of massive, early-type stars have been inspected in recent years in the search for sites where particles can be accelerated up to relativistic energies. Wind regions o…

astro-ph.HE2010★ 104 cited

Gamma rays from cloud penetration at the base of AGN jets

Anabella T. Araudo, Valenti Bosch-Ramon, Gustavo E. Romero

Dense and cold clouds seem to populate the broad line region surrounding the central black hole in AGNs. These clouds could interact with the AGN jet base and this could have obser…

astro-ph.HE2010★ 2 cited

High-energy emission from jet-cloud interactions in AGNs

Anabella T. Araudo, Valenti Bosch-Ramon, Gustavo E. Romero

Active galactic nuclei present continuum and line emission. The emission lines are originated by gas located close to the central super-massive black hole. Some of these lines are…