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On the Methanol masers in G9.62+0.20E: Preliminary colliding-wind binary (CWB) calculations

  • S. P. van den Heever (a1), D. J. van der Walt (a1), J. M. Pittard (a2) and M. G. Hoare (a2)
Abstract
Abstract

A 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.

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      On the Methanol masers in G9.62+0.20E: Preliminary colliding-wind binary (CWB) calculations
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References
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Goedhart S., Gaylard M., & van der Walt D. J. 2003, MNRAS, 333, L33L36
van der Walt D. J., Goedhart S., & Gaylard M. 2009, MNRAS, 398, 961970
van der Walt D. J. 2011, AJ, 141, 152
Stevens I. R., Blondin J. M., & Pollock A. M. T. 1992, APJ, 386, 265287
Sternberg A., Hoffmann T. L., & Pauldrach A. W. A. 2003, ApJ, 599, 13331343
Pittard J. M. & Stevens I. R. 1997, MNRAS, 292, 298
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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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