An orbital period analysis of the dwarf novae OY Carinae

Z.-T. HAN; S.-B. QIAN; E. FERNÁNDEZ LAJÚS; W.-P. LIAO; J. ZHANG

NEW ASTRONOMY

ELSEVIER SCIENCE BV

Lugar: Amsterdam; Año: 2015 vol. 34 p. 1 - 5

1384-1076

By using our twelve new CCD times of light minimum of OY Carinae (OY Car) together with those collected from the literature, it is found that the O?C curve of OY Car shows a downward parabola with an amplitude of 27.8 s and a cyclic change of a period 14.0 yr. The period decrease is opposite to the hypothesis of mass transfer, and it cannot be explained by angular momentum loss via gravitational radiation. The Rappaport et al. (1983)?s magnetic braking (MB) prescription is adopted to explain the observed orbital period decrease. The cyclic change of period is analyzed with the light travel-time effect that originates from gravitational influence of a third body. The mass of the third star is determined to be M3 sini = 0.008097(+-0.000014) Msol = 8.48(+-0.02) MJup, suggesting that it may be a critical substellar object between brown dwarf and giant planet. If the orbital inclination of the third body equals 90º, the distance between the third body and the mass centre of the whole system is about 6.18(+-0.45) AU.