SXP 15.6 – an accreting pulsar close to spin equilibrium?

ABSTRACT SXP 15.6  is a recently established Be star X-ray binary system in the Small Magellanic Cloud (SMC). Like many such systems, the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. It is shown here that the neutron star in this system is exceptionally cl...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2022-05, Vol.513 (4), p.5567-5574
Hauptverfasser:	Coe, M J, Monageng, I M, Kennea, J A, Buckley, D A H, Evans, P A, Udalski, A, Groot, Paul, Bloemen, Steven, Vreeswijk, Paul, McBride, Vanessa, Klein-Wolt, Marc, Woudt, Patrick, Körding, Elmar, Le Poole, Rudolf, Pieterse, Danielle
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!