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 \times 10 ^ { -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 \geq 0.20 ) 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 .