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Molecular Gas Around the Infrared Dust Bubbles

Published online by Cambridge University Press:  21 March 2013

Yan Gong
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, West Beijing Road, Nanjing 210008, China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences University of Chinese Academy of Sciences email: [email protected]
Ruiqing Mao
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, West Beijing Road, Nanjing 210008, China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences
Min Fang
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, West Beijing Road, Nanjing 210008, China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences
Jixian Sun
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, West Beijing Road, Nanjing 210008, China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences
Dengrong Lu
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, West Beijing Road, Nanjing 210008, China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences
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Abstract

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We have conducted a mapping survey toward a sample of 17 infrared dust bubbles in three 3 mm waveband CO isotopic lines simultaneously. Such bubbles are candidates to search for triggered massive star formation. We present the data and report preliminary results.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

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