Non-thermal processes in bowshocks of runaway stars: Application to ζ Ophiuchi

Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to the interstellar medium. These stars can produce bowshocks in the surrounding gas. Bowshocks develop as arc-shaped structures, with bows pointing to the same direction as the stellar velocity, while th...

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Detalles Bibliográficos
Autores principales:	Valle, María Elena del, Romero, Gustavo Esteban
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas Gamma rays: general ISM: jets and outflows Radiation mechanisms: non-thermal Stars: early-type Stars: individual:ζOphiuchi
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84645
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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