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A study of the infrared emission of three H II regions S 140–142 |
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| Authors: | Jin-zeng Li Pei-sheng Chen |
| Affiliation: | 1 Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China 2 Joint Laboratory for Optical Astronomy, Chinese Academy of Sciences, Beijing 100080, China 3 Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China |
| Abstract: | The infrared emission of the H II region-molecular cloud complexes S 140, S 141 and S 142 is examined using the IRAS Sky Survey Atlases. The IRAF and Skyview software are used to draw the contour maps of infrared intensity, color temperature and optical depth of each source. The total infrared luminosity and dust distribution in the complexes are given. Compact clumps where star formation probably takes place are identified. The exciter star of S 141 is analyzed. |
| Keywords: | ISSA interstellar matter H II region molecular cloud |
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