Circumbinary Planets Orbiting the Rapidly Pulsating Subdwarf B-type binary NY Vir

QIAN S.-B.; ZHU L.-Y.; DAI Z.-B.; FERNÁNDEZ LAJÚS, E.; XIANG F.-Y.; HE, J.-J.

The Astrophysical Journal Letters

IOP Science

Año: 2012 vol. 745 p. 1 - 5

2041-8205

We report here the tentative discovery of a Jovian planet in orbit aroundthe rapidly pulsating subdwarf B-type (sdB-type) eclipsing binary NY Vir. By using new determined eclipse times together those collected from the literature, we detect that the observed-calculated (O-C) curve of NY Vir shows a small-amplitude cyclic variation with a period of 7.9 years and a semiamplitude of 6.1 s, while it undergoes a downward parabolic change (revealing a period decrease at a rate of _dP/dt = -9.2 x 10^-12). The periodic variation was analyzed for the light-travel time effect via the presence of a third body. The mass of the tertiary companion was determined to be M3 sin i´ = 2.3(+/-0.3) MJupiter when a total mass of 0.60 Msun for NY Vir is adopted. This suggests that it most probably is a giant circumbinary planet orbiting NY Vir at a distance of about 3.3 astronomical units (AU). Since the rate of period decrease can not be explained by true angular momentum loss caused by gravitational radiation or/and magnetic braking, the observed downward parabolic change in the O-C diagram may be only a part of a long-period (longer than 15 years) cyclic variation, which may reveal the presence of another Jovian planet (about 2.5 MJupiter) in the system.