Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S287(8), p. 112-113, 2012
DOI: 10.1017/s174392131200676x
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On the Methanol masers in G9.62+0.20E: Preliminary colliding-wind binary (CWB) calculations
Journal article published in 2012 by
S. P. van den Heever,
D. J. van der Walt 
,
J. M. Pittard,
M. G. Hoare
,
J. M. Pittard,
M. G. Hoare
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractA comparison between the observed periodic flaring of methanol maser sources in the star forming region G9.62+0.20E and the continuum emission from parts of a background HII region is made. Using a colliding wind binary (CWB) model preliminary calculations show that the CWB model results fit the maser light curves very well.
