X-raying the wind-wind collisions in HD 168112 and HD 167971

The O-type long-period binary HD 168112 and triple HD 167971 star systems have been known for several decades for their non-thermal synchrotron radio emission. This emission arises from relativistic electrons accelerated in the hydrodynamic shocks of the wind collisions in these systems. Such wind c...

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Veröffentlicht in:	arXiv.org 2024-10
Hauptverfasser:	Rauw, Gregor, Blomme, Ronny, Nazé, Yaël, Volpi, Delia
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Collisions Radio emission Stellar systems XMM (spacecraft)
Online-Zugang:	Volltext
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