No CrossRef data available.
Article contents
Molecular clouds in the Extreme Outer Galaxy
Published online by Cambridge University Press: 16 July 2018
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
More than 200 molecular clouds were newly found distributed beyond the Outer arm in the extreme outer Galaxy (EOG) region by MWISP. Those MCs roughly following the HI′s distribution well delineate the outermost spiral structure (the Outer Scutum-Centaurus arm) and warp of our Galaxy. Besides, those MCs show different σv-Radius relation and exhibit higher value of αvir than MCs in the inner Galaxy.
- 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. 187 - 188
- Copyright
- Copyright © International Astronomical Union 2018
References
Sun, Y., Xu, Y., Yang, J., Li, F. C., Du, X. Y., Zhang, S. B., & Zhou, X., 2015, ApJ, 798, L27Google Scholar
Sun, Y., Su, Y., Zhang, S. B., Xu, Y., Chen, X. P., Yang, J., Jiang, Z. B., & Fang, M., 2017, ApJS, 230, 17Google Scholar
You have
Access