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Star Formation in Molecular Cloud Associated with IRAS |
| QIN Sheng-Li1; WU Yue-Fang2;WANG Jun-Jie1;ZHAO Gang1;SHI Jian-Rong1;MARTIN Miller3 |
| 1National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012
2Department of Astronomy, Peking University, Beijing 100871
3Institute of Physics, Cologne University, Cologne 50937, Germany |
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| Cite this article: |
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QIN Sheng-Li, WU Yue-Fang, WANG Jun-Jie et al 2004 Chin. Phys. Lett. 21 1677-1680 |
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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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| Keywords:
98.38.-j
98.38.Dq
97.10.Bt
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Published: 01 August 2004
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| PACS: |
98.38.-j
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(Interstellar medium (ISM) and nebulae in Milky Way)
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98.38.Dq
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(Molecular clouds, H2 clouds, dense clouds, and dark clouds)
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97.10.Bt
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(Star formation)
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