@article{CamposPelisoliKamannetal.2018,
  author    = {Campos, Fabiola and Pelisoli, Ingrid Domingos and Kamann, Sebastian and Husser, T. -O. and Dreizler, S. and Bellini, A. and Robinson, E. L. and Nardiello, Domenico and Piotto, G. and Kepler, S. O. and Istrate, A. G. and Winget, D. E. and Montgomery, M. H. and Dotter, A.},
  title     = {Outliers},
  series = {Monthly notices of the Royal Astronomical Society},
  volume    = {481},
  journal   = {Monthly notices of the Royal Astronomical Society},
  number    = {4},
  publisher = {Oxford Univ. Press},
  address   = {Oxford},
  issn      = {0035-8711},
  doi       = {10.1093/mnras/sty2591},
  pages     = {4397 -- 4409},
  year      = {2018},
  abstract  = {We use Hubble Space Telescope multicolour photometry of the globular cluster 47 Tucanae to uncover a population of 24 objects with no previous classification that are outliers from the single-star model tracks in the colour-magnitude diagram and yet are likely cluster members. By comparing those sources with evolutionary models and X-ray source catalogues, we were able to show that the majority of those sources are likely binary systems that do not have any X-ray source detected nearby, most possibly formed by a white dwarf and a main-sequence star and a small number of possible double-degenerate systems.},
  language  = {en}
}