We report the discovery of two giant planets orbiting the K giant HD 33844 based on radial velocity data from three independent campaigns. The planets move on nearly circular orbits with semimajor axes AU and AU, and have minimum masses (m sin i) of and . Detailed N-body dynamical simulations show that the two planets have remained on stable orbits for more than 106 years for low eccentricities and are most likely trapped in a mutual 3:5 mean motion resonance.
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机译：我们报告了来自三个独立战役的径向速度数据，发现了两个绕着K巨人HD 33844旋转的巨型行星的发现。行星在具有半长轴AU和AU的近圆形轨道上运动，并且具有和的最小质量（m sin i）。详细的N体动力学模拟表明，由于低偏心率，两颗行星在稳定轨道上保持了106年以上，最有可能陷入相互3：5的平均运动共振中。
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