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OBSERVATIONS OF INTERSTELLAR WATER VAPOR IN OUTFLOW REGIONS

机译:流出区星际水蒸气的观测

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摘要

We have observed the 1_(10)-1_(01) transition of interstellar water vapor near 557 GHz toward the three outflow sources NGC 2071, L1157, and NGC 1333 IRAS 4 using the Submillimeter Wave Astronomy Satellite. In each case, the observations reveal broad emission from water in the outflow accompanied by a narrow absorption feature at the velocity of the quiescent gas. Our estimates of the average ortho-water abundance within the outflowing gas lie in the range (0.5-1.6) x 10~(-6) relative to H_2.
机译:我们已经使用亚毫米波天文学卫星观测到557 GHz附近星际水蒸气向三个流出源NGC 2071,L1157和NGC 1333 IRAS 4的1_(10)-1_(01)过渡。在每种情况下,观测结果都表明流出水中的水排放量大,同时在静态气体的速度下吸收特征较窄。相对于H_2,我们估算的流出气体中平均原水丰度在(0.5-1.6)x 10〜(-6)范围内。

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