Abstract
An extensive search for new methanol sources were made. Three new masers in the 70-61A+ transition and twenty-four new thermal sources in the 10−00A+ transition were detected. Our results support the idea that high- velocity flows may increase the abundance of methanol and that methanol masers arise in methanol-rich sources.
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© 1993 Springer-Verlag
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Kalenskii, S.V. et al. (1993). A study of methanol masers at 36 and 44 GHz and 48 GHz thermal emission around them. In: Clegg, A.W., Nedoluha, G.E. (eds) Astrophysical Masers. Lecture Notes in Physics, vol 412. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-56343-1_240
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DOI: https://doi.org/10.1007/3-540-56343-1_240
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