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Trigonometric Parallax of RCW 122
Wu, Y. W. ; Xu, Y. ; Menten, K. M. ; Zheng, X. W. ; Reid, M. J.
2012
Source PublicationCosmic Masers - from OH to H0, Proceedings of the International Astronomical Union, IAU Symposium
Volume287Pages:425-426
AbstractAs a part of the BeSSeL (Bar and Spiral Structure Legacy) survey, we report a trigonometric parallax for the massive star-forming region G348.70-1.04. Its distance is 3.38-0.27 +0.33 kpc, indicating that it is in the Scutum-Centaurus arm. Its proper motion is -0.73 +/- 0.04 mas yr-1 toward the east and -2.83 +/- 0.50 mas yr-1 toward the north.
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8120
Collection紫金山天文台青海观测站
Recommended Citation
GB/T 7714
Wu, Y. W.,Xu, Y.,Menten, K. M.,et al. Trigonometric Parallax of RCW 122[J]. Cosmic Masers - from OH to H0, Proceedings of the International Astronomical Union, IAU Symposium,2012,287:425-426.
APA Wu, Y. W.,Xu, Y.,Menten, K. M.,Zheng, X. W.,&Reid, M. J..(2012).Trigonometric Parallax of RCW 122.Cosmic Masers - from OH to H0, Proceedings of the International Astronomical Union, IAU Symposium,287,425-426.
MLA Wu, Y. W.,et al."Trigonometric Parallax of RCW 122".Cosmic Masers - from OH to H0, Proceedings of the International Astronomical Union, IAU Symposium 287(2012):425-426.
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