Hard X-ray cataclysmic variables

D. de Martino, F. Bernardini, K. Mukai, M. Falanga, N. Masetti

Resultado de la investigación: Contribución a una revistaArtículo

Resumen

Among hard X-ray Galactic sources detected with the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have surprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic Variables of the Intermediate Polar type, suggesting this subclass as an important constituent of the Galactic population of X-ray sources. We here review and discuss the X-ray emission properties of newly discovered sources in the framework of an identification programme with the XMM-Newton satellite that increased the sample of this subclass by a factor of two.

Idioma originalInglés
PublicaciónAdvances in Space Research
DOI
EstadoEn prensa - 1 ene 2019

Áreas temáticas de ASJC Scopus

  • Ingeniería aeroespacial
  • Astronomía y astrofísica
  • Geofísica
  • Ciencias atmosféricas
  • Ciencias planetarias y espacial
  • Ciencias planetarias y de la Tierra (todo)

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    de Martino, D., Bernardini, F., Mukai, K., Falanga, M., & Masetti, N. (Aceptado/En prensa). Hard X-ray cataclysmic variables. Advances in Space Research. https://doi.org/10.1016/j.asr.2019.09.006