Hellier & Beardmore 2002

Bibinfo (this paper at ADS): Hellier, C., Beardmore, A.P. 2002, MNRAS 331, 407-416.
Type: Observational: X-ray and optical spectroscopy.
Object(s): V2400 Oph.
Results: X-rays are dominated by sideband, spin and orbital pulses are very weak. Emission lines are consistent with stream-fed accretion model. This system is diskless, at very low (~10^o) inclination, but there is material that circles the white dwarf.

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