Volume 11 Issue 1
Jan.  1991
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Zheng Xing-wu. OH MASERS IN W33B[J]. Chinese Journal of Space Science, 1991, 11(1): 1-8. doi: 10.11728/cjss1991.01.001
Citation: Zheng Xing-wu. OH MASERS IN W33B[J]. Chinese Journal of Space Science, 1991, 11(1): 1-8. doi: 10.11728/cjss1991.01.001

OH MASERS IN W33B

doi: 10.11728/cjss1991.01.001 cstr: 32142.14.cjss1991.01.001
  • Received Date: 1989-09-18
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1991-01-24
  • The polarization observations are carried out towards OH masers in W33B with the 23/2, J = 3/2, F=1→1, and F = 2→2 transitions. The magnetic strength of 5 mGis inferred by the Zeeman splitting between right and left circular polarization spectra. The hydrogen density of the protostellar matter, n(H2) =3×107cm-3, in the active massing region is estimated by considering a spherical maser with the fully saturation and the homogeneous pumping.

     

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