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We report 18 new primary minima timing observations of the short-periodeclipsing binary system NY Virginis. We combined these minima with previouslypublished primary minima to update circumbinary exoplanet models in this systembased on O-C timing variations. We performed a non-linear least-squaresminimization search using a quadratic ephemeris and either one or twoexoplanets. 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 orbitstability shows that this solution is stable for at least $10^8$ yr, but asmall increase in eccentricity ($e\geq0.20$) for either planet renders theorbits unstable in less than $10^6$ years. A number of model parameters aresignificantly degenerate, so additional observations are required to determineplanetary parameters with high statistical confidence.

NY Vir Eclipse timing observations: Two planet solution