Star Formation in Molecular Cloud Associated with IRAS
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Abstract
The first mapping observations in 12CO J=2-1 and 12CO 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.
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QIN Sheng-Li, WU Yue-Fang, WANG Jun-Jie, ZHAO Gang, SHI Jian-Rong, MARTIN Miller. Star Formation in Molecular Cloud Associated with IRAS[J]. Chin. Phys. Lett., 2004, 21(8): 1677-1680.
QIN Sheng-Li, WU Yue-Fang, WANG Jun-Jie, ZHAO Gang, SHI Jian-Rong, MARTIN Miller. Star Formation in Molecular Cloud Associated with IRAS[J]. Chin. Phys. Lett., 2004, 21(8): 1677-1680.
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QIN Sheng-Li, WU Yue-Fang, WANG Jun-Jie, ZHAO Gang, SHI Jian-Rong, MARTIN Miller. Star Formation in Molecular Cloud Associated with IRAS[J]. Chin. Phys. Lett., 2004, 21(8): 1677-1680.
QIN Sheng-Li, WU Yue-Fang, WANG Jun-Jie, ZHAO Gang, SHI Jian-Rong, MARTIN Miller. Star Formation in Molecular Cloud Associated with IRAS[J]. Chin. Phys. Lett., 2004, 21(8): 1677-1680.
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