  We report 18 new primary minima timing observations of the short-period
eclipsing binary system NY Virginis. We combined these minima with previously
published primary minima to update circumbinary exoplanet models in this system
based on O-C timing variations. We performed a non-linear least-squares
minimization search using a quadratic ephemeris and either one or two
exoplanets. The only model with an acceptable fit includes a period derivative
$\dot{P} = 2.83\times10^{-12}$ and two planets in eccentric orbits $e =
0.15,0.15$ with minimum masses 2.7 and 5.5 Jovian masses. Analysis of the orbit
stability shows that this solution is stable for at least $10^8$ yr, but a
small increase in eccentricity ($e\geq0.20$) for either planet renders the
orbits unstable in less than $10^6$ years. A number of model parameters are
significantly degenerate, so additional observations are required to determine
planetary parameters with high statistical confidence.
