Volume 14 Issue 3
Aug.  1994
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Zheng Xing-wu. OH MASERS IN W33A[J]. Chinese Journal of Space Science, 1994, 14(3): 177-182. doi: 10.11728/cjss1994.03.177
Citation: Zheng Xing-wu. OH MASERS IN W33A[J]. Chinese Journal of Space Science, 1994, 14(3): 177-182. doi: 10.11728/cjss1994.03.177

OH MASERS IN W33A

doi: 10.11728/cjss1994.03.177 cstr: 32142.14.cjss1994.03.177
  • Received Date: 1993-08-03
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1994-08-24
  • The circular polarization spectra in W33A are observed on emission from the 23/2 J=3/2, F=1→1 and F=2→2 transition of OH. The hydrogen density in the masing region is infered about 107 cm-3 in both the long thin tube and spherical maser,Apump rate of ~1(OH) cm-3s-1 is required in both geometries for the photon emission rate of ~1046s-1. The required pump efficiency is higher in the sphericalmaserthan in the thin tube.

     

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