The donor of Aquila X-1 revealed by high-angular resolution near-infrared spectroscopy

The low-mass X-ray binary Aquila X-1 is one of the most active neutron star X-ray transients. Despite its relatively bright quiescent optical counterpart, the detection of its companion has been hampered by the presence of a nearby interloper star. Using the Spectrograph for INtegral Field Observati...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society. Letters 2017-01, Vol.464 (1), p.L41-L45
Hauptverfasser:	Mata Sánchez, D., Muñoz-Darias, T., Casares, J., Jiménez-Ibarra, F.
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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