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Water Masers Toward Star-Forming Regions in the Bolocam Galactic Plane Survey

机译:在博洛姆银河普林飞机调查中朝向星形区域的水粉

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We present preliminary results of a search for 22 GHz water masers toward 1400 star-forming regions seen in the Bolocam Galactic Plane Survey (BGPS) using the Green Bank Telescope (GBT). The BGPS is a blind survey of the Northern Galactic plane in 1.1 mm thermal dust emission that has cataloged star-forming regions at all evolutionary stages. Further information is required to determine the stage of each BGPS source. Since water masers are produced by outflows from low and high-mass star forming regions, their presence is a key component of determining whether the BGPS sources are forming stars and which evolutionary stage they are in. We present preliminary detection statistics, basic properties of the water masers, and correlations with physical properties determined from the 1.1 mm emission and ammonia observations obtained concurrently with the water masers on the GBT.
机译:我们使用绿色银行望远镜(GBT)来提出22个GHz水粉的搜索结果朝向Bolocam Balactic Plane Square(BGPS)中的1400个星形地区。 BGPS是对1.1毫米热粉尘发射的北半空星平面的盲目调查,其在所有进化阶段都具有编目的星形区域。需要进一步的信息来确定每个BGPS源的阶段。由于水粉用水粉丝由来自低质量和大质量的星形形成区域的流出产生,因此它们的存在是确定BGPS源是形成恒星的关键组分,它们是否存在进化阶段。我们呈现初步检测统计数据,基本属性水式用具和与从GBT上的水粉同时获得的1.1mm发射和氨观察测定的物理性质的相关性。

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