[vsnet-chat 7869] paper: Intermediate Polar V405 Aur: Low-Mass Third Body or Precession ?

[Ivan Andronov]

2013arXiv1306.4665B

Variability of the Spin Period of the White Dwarf in the Intermediate Polar V405 Aur: Low-Mass Third Body or Precession ?

Breus, V. V.; Andronov, I. L.; Dubovsky, P.; Kolesnikov, S. V.; Zhuzhulina, E. A.; Hegedus, T.; Beringer, P.; Petrik, K.; Robertson, J. W.; Kudzej, I.; Shakhovskoy, N. M.

"Journal of Physical Studies", 2013

We present the results of photometric CCD observations of the magnetic cataclysmic variable V405 Aurigae (RX J0558.0+5353 = 1RXS J055800.7+535358) obtained using different instruments. We analysed variability of the spin period of the white dwarf in the V405 Aur (RX J0558.0+5353) system using our observations and previously published maxima timings. The spin period of the system in 2010-2012 is $P=545.4558163(94)$s. As we have gaps in observational data, we present 2 hypotheses of the spin period variability of this system - a cubic ephemeris which may be interpreted by a precession of the magnetic white dwarf or a periodic change with a period of 6.2 years and semi-amplitude of $17.2\pm1.8$ sec. The periodic variations may be interpreted by a light-time effect caused by a low-mass star ($M_3\ge0.09M_\odot$). In this case, the system belongs to a rare class of cataclysmic variables with a third body.