On the Methanol masers in G9.62+0.20E: Preliminary colliding-wind binary (CWB) calculations
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.
- Publication:
-
Cosmic Masers - from OH to H0
- Pub Date:
- July 2012
- DOI:
- 10.1017/S174392131200676X
- Bibcode:
- 2012IAUS..287..112V
- Keywords:
-
- masers;
- hydrodynamics