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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References
Bachiller R., Menten K.M., Gomez-Gonzalez J., Barcia A. (1990), Astron. & Astrophys., 240, 115.
Fukui Y. in: ESO Workshop on Low Mass Star Formation and Pre-Main Sequence Objects, (1989), 11–13 Jul., ed. R.Reipurth, 95–117.
Haschick A.D., Menten K.M., Baan W.A. Astrophys. J., (1990), 354, 555.
Menten K. M. Walmsley C. M., Henkel C., Wilson T. L.Astron.&Astrophys., (1988), 198, 253.
Morimoto M., Ohishi M., Kanzava T. Astrophys. J., (1985), 288, L11.
Plambeck R. L., Menten K. M.Astrophys.J., (1990), 364, 555.
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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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