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新外向流源S 146和IRAS 23545 6508
引用本文:杨传义,吴月芳.新外向流源S 146和IRAS 23545 6508[J].中国天文和天体物理学报,1998(3).
作者姓名:杨传义  吴月芳
作者单位:北京大学地球物理系
摘    要:用紫金山天文台青海观测站137m射电望远镜对S146和IRAS23545+6508进行了12CO(J=1-0)谱线的成图观测,结果表明两源附近存在CO高速外向流.分析了这两个外向流的形态,求出了其物理和动力学参数,同时结合IRAS资料,对中心源的演化阶段和环境气体的热特性作了分析.

关 键 词:星际分子  喷流和外向流  恒星形成

New Molecular Outflow Sources:S 146 and IRAS 23545 6508
YANG Chuan-yi,WU Yue-fang.New Molecular Outflow Sources:S 146 and IRAS 23545 6508[J].Chinese Journal of Astronomy and Astrophysics,1998(3).
Authors:YANG Chuan-yi  WU Yue-fang
Abstract:A 12 CO( J =1-0)line-mapping observation using the newly built 3mm system of the 13 7m radio telescope at the Qinghai Station of Purple Mountain Observatory showed there are high velocity molecular outflows near IRAS 22475 5939(S 146)and 23545 6508.The morphologies of the two outflows are analyzed and their physical and dynamical parameters are calculated and discussed.Using the IRAS data,the evolutionary status of the central sources and the thermal characteristics of the ambient gas are also investigated.
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