Abstracto
- We present Very Large Array (VLA) observations of the 70–61A+ methanol maser transition at 44 GHz toward NGC 6334F, G8.67−0.36, and M17. These arcsecond resolution observations complete a previous, larger VLA survey of this maser transition in high-mass, star-forming regions reported by Kurtz et al. We confirm the presence of 44 GHz methanol maser emission in all 3 sources, detecting 8 distinct maser components in NGC 6334F, 12 components in G8.67−0.36, and 1 in M17.