Star Formation in Molecular Cloud Associated with IRAS 07028-1100

Details Star Formation in Molecular Cloud Associated with IRAS 07028-1100 Star Formation in Molecular Cloud Associated with IRAS 07028-1100

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004chphl..21.1677q&link_type=abstract

Chinese Physics Letters, Volume 21, Issue 8, pp. 1677-1680 (2004).

Physics

Scientific paper

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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