Is Nova Centauri 1986 an "X-ray-quiet'' intermediate polar?

Details Is Nova Centauri 1986 an "X-ray-quiet'' intermediate polar? Is Nova Centauri 1986 an "X-ray-quiet'' intermediate polar?

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..117l&link_type=abstract

XMM-Newton Proposal ID #06532801

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, V842 Cen

Scientific paper

V842 Cen underwent a nova eruption in 1986 and in 2008 a period of 57 s has been detected in optical photometry, likely related with the white dwarf spin making the system a strong candidate of the intermediate polar class. We propose to use the unique capabilities of XMM-Newton to search for X-ray emission and characterize the accretion process onto the likely magnetized white dwarf.

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