Hard X-ray cataclysmic variables

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

Resultado de la investigación: Article

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 originalEnglish
PublicaciónAdvances in Space Research
DOI
EstadoAccepted/In press - 1 ene 2019

Huella dactilar

cataclysmic variables
X rays
x rays
XMM-Newton telescope
newton
Satellites

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

Citar esto

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
de Martino, D. ; Bernardini, F. ; Mukai, K. ; Falanga, M. ; Masetti, N. / Hard X-ray cataclysmic variables. En: Advances in Space Research. 2019.
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de Martino, D, Bernardini, F, Mukai, K, Falanga, M & Masetti, N 2019, 'Hard X-ray cataclysmic variables', Advances in Space Research. https://doi.org/10.1016/j.asr.2019.09.006

Hard X-ray cataclysmic variables. / de Martino, D.; Bernardini, F.; Mukai, K.; Falanga, M.; Masetti, N.

En: Advances in Space Research, 01.01.2019.

Resultado de la investigación: Article

TY - JOUR

T1 - Hard X-ray cataclysmic variables

AU - de Martino, D.

AU - Bernardini, F.

AU - Mukai, K.

AU - Falanga, M.

AU - Masetti, N.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - 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.

AB - 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.

KW - Accretion

KW - Accretion discs

KW - Stars: cataclysmic variables

KW - X-Rays: binaries

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JF - Advances in Space Research

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de Martino D, Bernardini F, Mukai K, Falanga M, Masetti N. Hard X-ray cataclysmic variables. Advances in Space Research. 2019 ene 1. https://doi.org/10.1016/j.asr.2019.09.006