Evidence of non-thermal x-ray emission from HH 80

Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emi...

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Detalles Bibliográficos
Autores principales:	López Santiago, J., Peri, Cintia Soledad, Bonito, R., Miceli, M., Albacete Colombo, Juan Facundo, Benaglia, Paula, De Castro, E.
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2013
Materias:	Ciencias Astronómicas Herbig-Haro objects ISM: jets and outflows radiation mechanisms: non-thermal stars: individual
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85485
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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