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SMA, VLA and VLBA observations in a 105 L⊙ high mass star formation region IRAS 18360-0537

Published online by Cambridge University Press:  16 July 2018

Gang Wu ,
Keping Qiu ,
Jarken Esimbek  and
Xingwu Zheng
Gang Wu
Affiliation:
Xinjiang Astronomical Observatory, Chinese Acadmy of Sciences, Science 1-street 150, Beijing Road, Urumuqi, P. R. China, email: wug@xao.ac.cn School of Astronomy and Space Science, Nanjing University, Nanjing 210093, P. R. China Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Urumqi 830011, P. R. China University of the Chinese Academy of Sciences, Beijing 100080, P. R. China
Keping Qiu
Affiliation:
School of Astronomy and Space Science, Nanjing University, Nanjing 210093, P. R. China
Jarken Esimbek
Affiliation:
Xinjiang Astronomical Observatory, Chinese Acadmy of Sciences, Science 1-street 150, Beijing Road, Urumuqi, P. R. China, email: wug@xao.ac.cn University of the Chinese Academy of Sciences, Beijing 100080, P. R. China
Xingwu Zheng
Affiliation:
School of Astronomy and Space Science, Nanjing University, Nanjing 210093, P. R. China
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Abstract

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We have observed a young stellar object, IRAS 18360-0537, with a far-infrared luminosity of 1.2 × 105 L⊙. It is perhaps the most promising candidate of a high-mass protostar associated with a Keplerian disk and a jet/outflow system in the regime of L > 105L⊙. We are conducting the SMA, VLA, and VLBA studies to provide a comprehensive understanding of this interesting high mass star formation scenario.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 291 - 292
Copyright
Copyright © International Astronomical Union 2018 

References

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