η Carinae with Fermi -LAT: two full orbits and the third periastron

Context. Colliding-wind binaries are massive stellar systems featuring strong, interacting winds. These binaries may be actual particle accelerators, making them variable γ -ray sources due to changes in the wind collision region along the orbit. However, only two of these massive stellar binary sys...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-10, Vol.654, p.A44
Hauptverfasser:	Martí-Devesa, G., Reimer, O.
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Gamma emission Gamma ray sources Orbits Particle accelerators Stellar systems Wind
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!