A search for optical counterparts in quiescent black hole X-ray transients

Dynamical mass measurements of compact stars in X-ray transients demand the detection of optical/near-infrared counterparts in quiescence. Out of the 73 black hole candidates in X-ray transients, optical and near-infrared quiescent counterparts have only been identified for 34 objects. We present UL...

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Auteurs principaux:	Yanes-Rizo I. V., Casares J., Torres M. A. P., Dhillon V. S., Marsh T. R., Armas Padilla M., Jonker P. G., Muñoz-Darias T., Navarro Umpiérrez S., Steeghs D.
Format:	Artigo
Langue:	Inglês
Publié:	EDP Sciences 2026-04-01
Collection:	Astronomy & Astrophysics
Sujets:	accretion accretion disks binaries: close stars: black holes
Accès en ligne:	https://www.aanda.org/articles/aa/full_html/2026/04/aa57696-25/aa57696-25.html
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