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A non-local model of line emission from molecular clouds

  • Part I: The Physics of Interstellar Molecular Clouds: Theory
  • Conference paper
  • First Online:
The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 331))

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Abstract

A technique developed by Scharmer & Carlsson for finding accurate solutions to the multi-level line transfer problem in the presence of velocity fields has been adapted for modelling the submillimetre emission spectra of molecular clouds. Line profiles for transitions up to J=20−19 in CO and J=5−4 in HCO+ can be modelled for slab or spherically symmetric atmospheres exhibiting spatial variations in temperature, density and bulk velocity. The technique is used to reproduce the published observed profiles of HCO+, CO and its isotopes, using a single physical model of the Bok globule B335.

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© 1989 Springer-Verlag Berlin Heidelberg

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Glasse, A.C.H. (1989). A non-local model of line emission from molecular clouds. In: The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics. Lecture Notes in Physics, vol 331. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0119506

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  • DOI: https://doi.org/10.1007/BFb0119506

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-51297-4

  • Online ISBN: 978-3-540-46187-6

  • eBook Packages: Springer Book Archive

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