Massive star-formation toward G28.87+0.07
Date Issued
2012
Author(s)
Li, J. J.
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Furuya, R. S.
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Xu, Y.
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Usuda, T.
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Menten, K. M.
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Pestalozzi, M.
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Abstract
We investigated the high-mass star-forming region G28.87+0.07 by means of maser kinematics, including H2O, CH3OH, and OH, and radio to infrared, continuum observations. All observational evidence suggests that these masers are associated with the same young star of 20-30 M⊙, still in the main accretion phase and surrounded by a rich stellar cluster.
Coverage
Cosmic Masers - from OH to H0
All editors
Booth, R.S.; Humphreys, E.M.L.; Vilemmings, W.H.T.
Volume
vol. 8, S287
Start page
180
Conferenece
Cosmic Masers - from OH to H0
Conferenece place
Stellenbosch, South Africa
Conferenece date
29 January- 3 February, 2012
Issn Identifier
1743-9213
Ads BibCode
2012IAUS..287..180L
Rights
open.access
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