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Star Formation in Molecular Cloud Associated with IRAS 07028-1100
作者姓名:秦胜利 吴月芳 王俊杰 赵刚 施建荣 MARTINMiller
作者单位:[1]NationalAstronomicalObservatories,ChineseAcademyofSciences,Beijing100012 [2]DepartmentofAstronomy,PekingUniversity,Beijing100871 [3]InstituteofPhysics,CologneUniversity,Cologne50937,Germany
摘    要:The first mapping observations in 12^CO J=2-1 and 12^CO J=1-0 lines were made towards molecular cloud associated with IRAS 07028-1100. The results show a mono-polar outflow (primarily blueshifted component) near IRAS 07028-1100, which suggests that star formation is occurring in this region. On the basis of the MSX (Midcourse Space Experiment) band-A image, molecular cloud core contours, NVSS data and IRAS data, we identify IRAS 07028-1100 as an embedded young intermediate-mass star. According to the 2MASS data, we suggest a sequential star formation in the infrared cluster associated with IRAS 07028-1100.

关 键 词:恒星形成 分子云 IRAS 07028-1100 天体观测 红外线束 NVSS数据
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