Origins of X-Ray Line Emissions in Circinus X-1 at Very Low X-Ray Flux

Accretion conditions and morphologies of X-ray transients containing neutron stars are still poorly understood. Circinus X-1 is an enigmatic case where we observe X-ray flux changes covering four orders of magnitude. We observed Circinus X-1 several times at its very lowest X-ray flux using the high...

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Veröffentlicht in:	The Astrophysical journal 2020-03, Vol.891 (2), p.150
Hauptverfasser:	Schulz, N. S., Kallman, T. E., Heinz, S., Sell, P., Jonker, P., Brandt, W. N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Accretion disks Astrophysics Binary stars Blackbody Companion stars Emission Emissions Energy transmission Field strength Fluctuations High mass x-ray binary stars Luminosity Magnetic fields Morphology Neutron flux Neutron stars Photoionization Space telescopes Stellar winds X ray binaries X ray sources X ray stars X ray telescopes X-ray bursts X-ray fluxes
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