Is the bowshock of the runaway massive star HD 195592 a Fermi source?

Context. HD 195592 is an O-type super-giant star, known as a well-established runaway. Recently, a Fermi γ-ray source (2FGL J2030.7+4417) with a position compatible with that of HD 195592 has been reported. Aims. Our goal is to explore the scenario where HD 195592 is the counterpart of the Fermi γ-r...

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Detalles Bibliográficos
Autores principales:	Valle, María Victoria del, Romero, Gustavo Esteban, De Becker, M.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2013
Materias:	Ciencias Astronómicas Gamma-rays: general Radiation mechanisms: non-thermal Stars individual: HD 195592 Stars: early-type
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85646
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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