We have obtained maps of the large-scale outflow associated with the UC H II region G5.89-0.39 in CO and 13CO (J = 3-2), SiO (J = 8-7, J = 5-4), SO2 (J = 132,12-131,13),13 and H13CO+(J = 4-3). From these maps we have been able to determine the mass (3.3 M☉), momentum (96 M☉ km s-1), energy (3.5 × 1046 ergs), mechanical luminosity (141 L☉), and mass-loss rate (~ 1 × 10-3 M☉ yr-1) in the large-scale outflow. The observationally derived parameters were used to guide three-dimensional magnetohydrodynamic models of the jet-entrained outflow. Through the combination of observations and simulations, we suggest that the large-scale outflow may be inclined by approximately 45° to the line of sight, and that the jet entraining the observed molecular outflow may have been active for as little as 1000 years, half the kinematic age of the outflow.
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机译：我们已经获得了与UC H II区G5.89-0.39在CO和13CO（J = 3-2），SiO（J = 8-7，J = 5-4），SO2相关的大规模流出图（J ＝ 132，12-131，13），13和H 13 CO +（J ＝ 4-3）。根据这些图，我们可以确定质量（3.3M☉），动量（96M☉km s-1），能量（3.5×1046 ergs），机械光度（141L☉）和质量损失率（ 〜1×10-3M☉yr-1）大规模流出。观测得出的参数被用来指导射流夹带流出的三维磁流体动力学模型。通过观察和模拟的结合，我们建议大规模流出可能相对于视线倾斜约45°，并且夹带观察到的分子流出的射流可能已经活跃了1000年，一半流出的运动年龄。
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