Add to ORKGThe young stellar object IRAS 16547-4247, identified with a massive protostar, presents a highly collimated wind which interacts with the environments. As a result, strong shocks are formed at the jet termination point and particles are accelerated there up to relativistic energies. In the present contribution, the high-energy emission due to non-thermal interactions is calculated.Fil: Araudo, Anabella Teresa. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires....
High-mass microquasars are binary systems consisting of a massive star and an accreting compact obje...
Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outf...
Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sourc...
Context: Massive stars form in dense and massive molecular cores. The exact formation mechanism is u...
In recent years, massive protostars have turned out to be a possible population of high-energy emitt...
Recent radio observations support a picture for star formation where there is accretion of matter on...
In recent years, massive protostars have turned out to be a possible population of high-energy emitt...
We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock wi...
Several binary systems hosting a massive star and a companion thatis either a similar star or a comp...
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, the...
Thermal radio and X-ray emission has been traditionally associated with the formation of stars. Howe...
Protostellar jets are present in the later stages of the stellarformation. Non-thermal radio emissio...
Context. Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. ...
Massive protostars have associated bipolar outflows with velocities of hundreds of km/s. Such outflo...
High-mass microquasars are binary systems consisting of a massive star and an accreting compact obje...
Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outf...
Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sourc...
Context: Massive stars form in dense and massive molecular cores. The exact formation mechanism is u...
In recent years, massive protostars have turned out to be a possible population of high-energy emitt...
Recent radio observations support a picture for star formation where there is accretion of matter on...
In recent years, massive protostars have turned out to be a possible population of high-energy emitt...
We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock wi...
Several binary systems hosting a massive star and a companion thatis either a similar star or a comp...
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, the...
Thermal radio and X-ray emission has been traditionally associated with the formation of stars. Howe...
Protostellar jets are present in the later stages of the stellarformation. Non-thermal radio emissio...
Context. Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. ...
Massive protostars have associated bipolar outflows with velocities of hundreds of km/s. Such outflo...
High-mass microquasars are binary systems consisting of a massive star and an accreting compact obje...
Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outf...
Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sourc...