Simulations of stellar/pulsar-wind interaction along one full orbit

Context. The winds from a non-accreting pulsar and a massive star in a binary system collide forming a bow-shaped shock structure. The Coriolis force induced by orbital motion deflects the shocked flows, strongly affecting their dynamics. Aims. We study the evolution of the shocked stellar and pulsa...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2012-08, Vol.544, p.A59
Hauptverfasser:	Bosch-Ramon, V., Barkov, M. V., Khangulyan, D., Perucho, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	gamma rays: stars hydrodynamics outflows radiation mechanisms: non-thermal stars: winds X-rays: binaries
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!