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A Model for the Maser Source NGC 7538 IRS 1
Published online by Cambridge University Press: 07 August 2017
Abstract
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High resolution observations of the molecular cloud around NGC 7538 IRS 1 in the J=1-0 transition of 13CO show that the lower bound for density in that region is about 2 × 103 cm−3. The study of various molecular transitions and the continuum measurements of the H II region indicate that the conditions required by the Boland and de Jong model for the excitation of the H2CO maser are not very stringent or unique.
- Type
- Chemistry of Interface Regions
- Information
- Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 347 - 348
- Copyright
- Copyright © Kluwer 1992
References
REFERENCES
Forster, J. R., Goss, W. M., Gardner, F. F., and Stewart, R. T.
1985,
M.N.R.A.S.
, 216, 35P.Google Scholar
Gardner, F. F., Whiteoak, J. B., Forster, J. R., and Pankonin, V.
1986,
M.N.R.A.S.
, 218, 385.Google Scholar
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