Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S242(3), p. 184-185, 2007
DOI: 10.1017/s1743921307012914
Full text: Unavailable
AbstractHigh angular resolution observations are essential for understanding the nature of maser emission and the sources which excite it. Here we present preliminary results from MERLIN observations of three methanol masers from the Toruń survey. These MERLIN observations are being analysed as part of the interferometric component of the Methanol Multibeam (MMB) Survey which is surveying the Galactic plane at |b|≤2° for 6.67 GHz methanol maser sources.