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Disk Outflow Models as Applied to High Mass Star Forming Regions through Methanol and Water Maser Observations

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Figure

Figure 1. Diagram showing the energy levels of type E methanol for different values of K, where K is the projection of the total angular momentum J onto the principal axes of the molecule
Figure 3 shows the Class II methanol maser and the Class I methanol maser in G9.62 + 0.19, together with other
Figure 3. Figure showing the Class II and the Class I methanol maser and other sources of interest in region G9.62 + 0.19
Table 1. Positions and associated information for sources associated with G9.62 + 0.19
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