Abstract
All interstellar methanol maser sources can be divided into two classes. Their spectra are distinctive. In particular, the prominent Class II maser transitions, 6.7GHz and 12.2GHz lines show enhanced absorption toward Class I sources. We notice that the 6.7 and 12.2GHz methanol masers toward Class II sources are associated with each other and coexist toward ultracompact HII regions. Therefore we suggest a new pumping mechanism – methanol masers without population inversion. It can be used to explain the formation of 6.7GHz methanol masers while the 12.2GHz methanol masers are regarded as driving coherent microwave field. In this paper, we demonstrate that the new mechanism is associated with astronomical conditions and does not contradict with other mechanisms.
Similar content being viewed by others
References
Anderson, T.: 1992, Astrophys. J. Suppl. 82, 405.
Batral, W., et al.: 1987, Nature 326, 49.
Dijkerman, H.A. and Dynamus, A.: 1962, Physica 28, 977.
Elitzur, M.: 1992, Astrophysical Masers, Kluwer Academic Publishers.
Lees, R.M. and Hague, S.S.: 1974, Can. J. Phys. 52, 2250.
Fearn, H., et al.: 1992, Optics Comm. 87, 323.
Menten, K.M.: 1991a, in: A.D. Haschick and P.T.P. Ho (eds.), Skylines, Proc. Third Haystack Observatory Meeting, ASP, San Francisco, 119.
Menten, K.M.: 1991b, Astrophys. J. 380, L75.
Menten, K.M.: 1992, in: A.W. Clegg and G.E. Nedoluha (eds.), Astrophysical Masers, Springer-Verlag.
Moruzzi, G., et al.: 1992, J. Mol. Spectrosc. 153, 511.
Moruzzi, G., et al.: 1994, J. Mol. Spectrosc. 167, 156.
Norris, S.P., et al.: 1992, in: A.W. Clegg and G.E. Nedoluha (eds.), Astrophysical Masers, Springer-Verlag.
Pei, C.C., et al.: 1988, Astron. Astrophys. Suppl. 76, 35.
Prasad, G.B., et al.: 1991, Optics Comm. 86,5, 409.
Sun, J., et al.: 1997, Acta Astron. Sin. 38(4), in press.
Walmsley, C.M., et al.: 1988, Astron. Astrophys. 197, 271.
Rights and permissions
About this article
Cite this article
Hanping, L., Jin, S. A Radiation Mechanism for Interstellar Methanol 6.7GHz Masers. Astrophysics and Space Science 253, 305–312 (1997). https://doi.org/10.1023/A:1000695517996
Issue Date:
DOI: https://doi.org/10.1023/A:1000695517996