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Methanol Maser Parallaxes and Proper Motions

Date Issued
2012
Author(s)
Xu, Y.
•
Reid, M. J.
•
•
Menten, K. M.
•
Zheng, X. W.
•
Brunthaler, A.
•
Zhang, B.
•
•
Li, J. J.
•
DOI
Abstract
Due to their compactness, persistence and slow motion, Class II CH3OH masers are excellent targets for parallax and proper motion measurements for massive star-forming regions in the Galactic Disk. These measurements can be used to improve our understanding of the spiral structure and dynamics of the Milky Way. At the same time, Class II CH3OH masers can also be used to study gas kinematics close to the exciting star, tracing rotation, infall and/or outflow motions.
Coverage
Cosmic Masers - from OH to H0
All editors
Booth, R.S.; Humphreys, E.M.L.; Vilemmings, W.H.T.
Series
Volume
vol. 8, S287
Start page
368
Conferenece
Cosmic Masers - from OH to H0
Conferenece place
Stellenbosch, South Africa
Conferenece date
29 January- 3 February, 2012
Uri
Url
Issn Identifier
1743-9213
Ads BibCode
2012IAUS..287..368X
Rights
open.access
File(s)
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Size

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Format

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