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Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020
J. M. Paredes, C. H. Ishwara-Chandra, V. Bosch-Ramon +3
There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to ident…
Relativistic stellar jets: dynamics and non-thermal radiation
V. Bosch-Ramon
Relativistic stellar jets, produced in binary systems called microquasars, propagate through media with different spatial scales releasing their energy in the form of work and radi…
Formation of large-scale magnetic structures associated with the Fermi bubbles
Maxim V. Barkov, Valenti Bosch-Ramon
The Fermi bubbles are part of a complex region of the Milky Way. This region presents broadband extended non-thermal radiation, apparently coming from a physical structure rooted i…
Clumpy stellar winds and high-energy emission in high-mass binaries hosting a young pulsar
V. Bosch-Ramon
High-mass binaries hosting young pulsars can be powerful gamma-ray emitters. The stellar wind of the massive star in the system is expected to be clumpy. Since the high-energy emis…
Gamma-ray emission from massive stars interacting with AGN jets
Anabella Araudo, Valenti Bosch-Ramon, Gustavo E. Romero
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermasive blac…
Studying the non-thermal lobes of IRAS 16547-4247 through a multi-wavelength approach
P. Munar-Adrover, V. Bosch-Ramon, J. M. Paredes +1
In the recent years massive protostars have been suggested to be high-energy emitters. Among the best candidates is IRAS 16547-4247, a protostar that presents a powerful outflow wi…