@article{08c90e4396264333a8acba3fd5e14749,
title = "Hard X-ray cataclysmic variables",
abstract = "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.",
keywords = "Accretion, Accretion discs, Stars: cataclysmic variables, X-Rays: binaries",
author = "{de Martino}, D. and F. Bernardini and K. Mukai and M. Falanga and N. Masetti",
note = "Funding Information: This work has been presented at the 42nd COSPAR Assembly in 2018 in Pasadena, USA, at the Session entitled ”Nova Eruptions, Cataclysmic Variables and related systems: Observational vs. theoretical challenges in the 2020 era. This work is based on data obtained with XMM-Newton and INTEGRAL , ESA science missions with instruments and contributions directly funded by ESA Member States, with Swift , a NASA science missions with Italian participation, with NuSTAR , a NASA science mission and with Gaia , an ESA mission, whose data are processed by the Data Processing and Analysis Consortium (DPAC). DdM acknowledges financial support from INAF-ASI agreement I/037/12/0 , ASI-INAF contract n. 2017-14-H.0 and INAF-PRIN SKA/CTA Presidential Decree 70/2016. FB is founded by the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement n. 664931 . NM acknowledges financial support from ASI-INAF contract n. 2017-14-H.0 . Funding Information: This work has been presented at the 42nd COSPAR Assembly in 2018 in Pasadena, USA, at the Session entitled ?Nova Eruptions, Cataclysmic Variables and related systems: Observational vs. theoretical challenges in the 2020 era. This work is based on data obtained with XMM-Newton and INTEGRAL, ESA science missions with instruments and contributions directly funded by ESA Member States, with Swift, a NASA science missions with Italian participation, with NuSTAR, a NASA science mission and with Gaia, an ESA mission, whose data are processed by the Data Processing and Analysis Consortium (DPAC). DdM acknowledges financial support from INAF-ASI agreement I/037/12/0, ASI-INAF contract n.2017-14-H.0 and INAF-PRIN SKA/CTA Presidential Decree 70/2016. FB is founded by the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement n. 664931. NM acknowledges financial support from ASI-INAF contract n.2017-14-H.0. Publisher Copyright: {\textcopyright} 2019 COSPAR",
year = "2020",
month = sep,
day = "1",
doi = "10.1016/j.asr.2019.09.006",
language = "English (US)",
volume = "66",
pages = "1209--1225",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier Limited",
number = "5",
}