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The synthesis of molecular line, neutral carbon and dust continuum observations in the molecular cloud G34.3+0.2

  • Star Formation in Molecular Clouds
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The Physics and Chemistry of Interstellar Molecular Clouds

Part of the book series: Lecture Notes in Physics ((LNP,volume 459))

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References

  • Heaton, B.D., Matthews, N., Little, L.T. and Dent, W.R.F., 1985. Mon. Not. R. Astron. Soc. 217, 485.

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  • Heaton, B.D., Little, L.T. and Bishop, I.S., 1989. Astron. Astrophys. 213, 148.

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  • Heaton, B.D., Little, L.T., Yamashita, T., Davies, S.R., Cunningham, C.T. and Monteiro, T.S., 1993. A&A 278, 238.

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  • Strong-Jones, F.S., Heaton, B.D. and Little, L.T., 1991, A&A 251, 263.

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Authors and Affiliations

  1. Electronic Eng. Laboratory, Univ. of Kent, CT2 7NT, Canterbury, Kent, UK

    L. T. Little

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  1. L. T. Little
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Gisbert Winnewisser Guido C. Pelz

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© 1995 Springer-Verlag

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Little, L.T. (1995). The synthesis of molecular line, neutral carbon and dust continuum observations in the molecular cloud G34.3+0.2. In: Winnewisser, G., Pelz, G.C. (eds) The Physics and Chemistry of Interstellar Molecular Clouds. Lecture Notes in Physics, vol 459. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102159

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  • DOI: https://doi.org/10.1007/BFb0102159

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-60482-2

  • Online ISBN: 978-3-540-47665-8

  • eBook Packages: Springer Book Archive

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