Broad-band spectral energy distribution of the X-ray transient Swift J1745−26 from outburst to quiescence

Aims. We aim to analyse our study of the X-ray transient Swift J1745−26, using observations obtained from its outburst in September 2012, up to its decay towards quiescence in March 2013. Methods. We obtained optical and infrared observations, through override programme at ESO/VLT with FORS2 and ISA...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-05, Vol.637, p.A2
Hauptverfasser:	Chaty, Sylvain, Fortin, Francis, López-Oramas, Alicia
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Accretion disks Astrophysics Binary stars Blackbody Companion stars Decay Deposition Domains Emission Infrared astronomy Light curve Luminosity Orbits Physics Radio Spectral energy distribution Synchrotrons X ray binaries X ray spectra X ray stars X-rays
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