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Further Microwave Emission Lines and Clouds of Ammonia in our Galaxy

Nature volume 221, pages 917–919 (1969)Cite this article

Abstract

Further NH3 emission has been found in the Sagittarius region, giving clues to the conditions in dust clouds.

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References

  1. Cheung, A. C., Rank, D. M., Townes, C. H., Thornton, D. D., and Welch, W. J., Phys. Rev. Lett., 21, 1701 (1968).

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  2. Cheung, A. C., Rank, D. M., Townes, C. H., Thornton, D. D., and Welch, W. J., Nature, 221, 626 (1969).

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Authors and Affiliations

  1. Department of Physics,

    A. C. CHEUNG, D. M. RANK & C. H. TOWNES

  2. Radio Astronomy Laboratory and Department of Electrical Engineering, University of California, Berkeley

    W. J. WELCH

Authors
  1. A. C. CHEUNG
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  2. D. M. RANK
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  3. C. H. TOWNES
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  4. W. J. WELCH
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CHEUNG, A., RANK, D., TOWNES, C. et al. Further Microwave Emission Lines and Clouds of Ammonia in our Galaxy. Nature 221, 917–919 (1969). https://doi.org/10.1038/221917a0

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  • DOI: https://doi.org/10.1038/221917a0

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