Add to ORKGSeveral binary systems hosting a massive star and a companion thatis either a similar star or a compact object, present non-thermal emission from radio to gamma-rays. This non-thermal emission is the consequence of the interactions of relativistic particles surrounded by the stellar wind. The main goal of this workis to characterize the high-energy physics of gamma-ray binaries by implementing ageneral modeling for their most important high-energy processes. To thoroughly investigate the effects of the emitter-star-observer geometry on the resultin gradiation, we sistematically applied a non-thermal leptonic model for different locations of the emitter, magnetic fields, and acceleration timescales. The results of this procedure are presente...
[eng] High-mass binary systems involve extreme environments that produce non-thermal emission from r...
Massive systems made of two or more stars are known to be the site for interesting physical processe...
In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact...
Context. Several binary systems hosting massive stars present gamma-ray emission. In most of these s...
Recent radio observations support a picture for star formation where there is accretion of matter on...
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, the...
Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outf...
In this paper, I present a general discussion of several astrophysical processes likely to play a ro...
Context. Recently, the colliding-wind region of the binary stellar system HD 93129A was resolved for...
Colliding winds of massive binaries have long been considered as potential sites of non-thermal high...
Context.Massive stars form in dense and massive molecular cores. The exact formation mechanism is un...
Colliding-wind massive star binaries are known to produce strong shocks in their wind-wind interacti...
La emisión gamma es la evidencia mas fuerte de que procesos no-térmicos tienen lugar en una fuente a...
The young stellar object IRAS 16547-4247, identified with a massive protostar, presents a highly col...
Thermal radio and X-ray emission has been traditionally associated with the formation of stars. Howe...
[eng] High-mass binary systems involve extreme environments that produce non-thermal emission from r...
Massive systems made of two or more stars are known to be the site for interesting physical processe...
In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact...
Context. Several binary systems hosting massive stars present gamma-ray emission. In most of these s...
Recent radio observations support a picture for star formation where there is accretion of matter on...
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, the...
Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outf...
In this paper, I present a general discussion of several astrophysical processes likely to play a ro...
Context. Recently, the colliding-wind region of the binary stellar system HD 93129A was resolved for...
Colliding winds of massive binaries have long been considered as potential sites of non-thermal high...
Context.Massive stars form in dense and massive molecular cores. The exact formation mechanism is un...
Colliding-wind massive star binaries are known to produce strong shocks in their wind-wind interacti...
La emisión gamma es la evidencia mas fuerte de que procesos no-térmicos tienen lugar en una fuente a...
The young stellar object IRAS 16547-4247, identified with a massive protostar, presents a highly col...
Thermal radio and X-ray emission has been traditionally associated with the formation of stars. Howe...
[eng] High-mass binary systems involve extreme environments that produce non-thermal emission from r...
Massive systems made of two or more stars are known to be the site for interesting physical processe...
In this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact...