@article{MathysKharchenkoHubrig1996,
  author    = {Mathys, Gautier and Kharchenko, N. and Hubrig, Swetlana},
  title     = {A kinematical study of rapidly oscillating Ap stars},
  year      = {1996},
  language  = {en}
}
@article{MathysHubrig1995,
  author    = {Mathys, Gautier and Hubrig, Swetlana},
  title     = {Magnetic fields of the HgMn spectros copic binaries chi Lup and 74 Aqr},
  year      = {1995},
  language  = {en}
}
@article{HubrigMathys1993,
  author    = {Hubrig, Swetlana and Mathys, Gautier},
  title     = {Mass loss, magnetic field and chemical inhomogenities in the he-weak star HD 21699},
  year      = {1993},
  language  = {en}
}
@article{HubrigMathys1995,
  author    = {Hubrig, Swetlana and Mathys, Gautier},
  title     = {Properties of HgMn spectroscopic binaries from high spectral resolution observations},
  year      = {1995},
  language  = {en}
}
@article{HubrigMathys1995,
  author    = {Hubrig, Swetlana and Mathys, Gautier},
  title     = {Some remarks on the origin of the abundance anomalies in HgMn stars},
  year      = {1995},
  language  = {en}
}
@misc{MorelCastroFossatietal.2014,
  author    = {Morel, T. and Castro, Norberto and Fossati, Luca and Hubrig, Swetlana and Langer, N. and Przybilla, Norbert and Sch{\"o}ller, Markus and Carroll, Thorsten Anthony and Ilyin, Ilya and Irrgang, Andreas and Oskinova, Lida and Schneider, Fabian R. N. and Simon D{\´i}az, Sergio and Briquet, Maryline and Gonz{\´a}lez, Jean-Francois and Kharchenko, Nina and Nieva, M.-F. and Scholz, Ralf-Dieter and de Koter, Alexander and Hamann, Wolf-Rainer and Herrero, Artemio and Ma{\´i}z Apell{\´a}niz, Jesus and Sana, Hugues and Arlt, Rainer and Barb{\´a}, Rodolfo H. and Dufton, Polly and Kholtygin, Alexander and Mathys, Gautier and Piskunov, Anatoly E. and Reisenegger, Andreas and Spruit, H. and Yoon, S.-C.},
  title     = {The B fields in OB stars (BOB) survey},
  series = {Postprints der Universit{\"a}t Potsdam : Mathematisch-Naturwissenschaftliche Reihe},
  journal   = {Postprints der Universit{\"a}t Potsdam : Mathematisch-Naturwissenschaftliche Reihe},
  number    = {821},
  issn      = {1866-8372},
  doi       = {10.25932/publishup-41523},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-415238},
  pages     = {8},
  year      = {2014},
  abstract  = {The B fields in OB stars (BOB) survey is an ESO large programme collecting spectropolarimetric observations for a large number of early-type stars in order to study the occurrence rate, properties, and ultimately the origin of magnetic fields in massive stars. As of July 2014, a total of 98 objects were observed over 20 nights with FORS2 and HARPSpol. Our preliminary results indicate that the fraction of magnetic OB stars with an organised, detectable field is low. This conclusion, now independently reached by two different surveys, has profound implications for any theoretical model attempting to explain the field formation in these objects. We discuss in this contribution some important issues addressed by our observations (e.g., the lower bound of the field strength) and the discovery of some remarkable objects.},
  language  = {en}
}
@article{HubrigMathys1994,
  author    = {Hubrig, Swetlana and Mathys, Gautier},
  title     = {The evolutionary state of magnetic Ap stars},
  year      = {1994},
  language  = {en}
}