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A multiwavelength study of the massive star-forming region IRAS 22506+5944

A multiwavelength study of the massive star-forming region IRAS 22506+5944
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摘要 We present a multi-line study of the massive star-forming region IRAS 22506+5944. A new 6.7 GHz methanol maser was detected. ^12CO, 13CO, C180 and HCO+ J = 1 - 0 transition observations reveal a star-formation complex consisting mainly of two cores. The dominant core has a mass of more than 200 Mo, while the other one is only about 35 340. Both cores are obviously at different evolutionary stages. A 12CO energetic bipolar outflow was detected with an outflow mass of about 15 Mo. We present a multi-line study of the massive star-forming region IRAS 22506+5944. A new 6.7 GHz methanol maser was detected. ^12CO, 13CO, C180 and HCO+ J = 1 - 0 transition observations reveal a star-formation complex consisting mainly of two cores. The dominant core has a mass of more than 200 Mo, while the other one is only about 35 340. Both cores are obviously at different evolutionary stages. A 12CO energetic bipolar outflow was detected with an outflow mass of about 15 Mo.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2009年第12期1343-1350,共8页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China(Grant Nos.10673024,10733030,10703010 and 10621303) the National Basic Research Program of China-973 Program(2007CB815403)
关键词 infrared: ISM - ISM: individual (IRAS 22506+5944) - ISM: jets andoutflows -- masers -- stars: formation infrared: ISM - ISM: individual (IRAS 22506+5944) - ISM: jets andoutflows -- masers -- stars: formation
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