Very high energy γ-ray emission from X-ray transients during major outbursts

Mostrar todas las versiones(2)

<b>Context.</b> Some high mass X-ray binaries (HMXB) have been recently confirmed as γ-ray sources by ground based Cherenkov telescopes. In this work, we discuss the γ-ray emission from X-ray transient sources formed by a Be star and a highly magnetized neutron star. This kind of systems...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Orellana, Mariana Dominga, Romero, Gustavo Esteban, Pellizza, L. J., Vidrih, S.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2007
Materias:
Ciencias Astronómicas
Gamma-rays: theory
Stars: individual: A0535+26
X-ray: binaries
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83002
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

Ejemplares similares

Ejemplares similares