The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X

An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, nonthermal emission processes such as inverse Compton (IC) scattering are expected to produce a high energy spectrum, in addition to the...

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Detalles Bibliográficos
Autores principales:	De Becker, M., Rauw, G., Pittard, J. M., Blomme, R., Romero, Gustavo Esteban, Sana, H., Stevens, I. R.
Formato:	Articulo Comunicacion
Lenguaje:	Inglés
Publicado:	2008
Materias:	Astronomía Ciencias Exactas Stars: early-type Radiation mechanisms: non-thermal X-rays: stars Acceleration of particles
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/96175 https://ri.conicet.gov.ar/11336/22954 http://sait.oat.ts.astro.it/MmSAI/79/PDF/242.pdf
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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