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.
References
Avrett, E.H., Loeser, R., in ‘Methods in Radiative Transfer’, C.U.P., ed. Kalkoffen, 341.
Draine, B.T., Roberge, W.G. 1984, Ap. J., 282, 491.
Flower, D.R., Launay, J.M. 1985, M.N.R.A.S., 214, 271.
Frerking, M.A., Langer, W.D., Wilson, R.W. 1987, Ap. J., 313, 320.
Glassgold, A.E., Huggins, P.J., Langer, W.D. 1985, Ap. J., 290, 615.
Goldreich, P., Kwan, J., 1974, Ap. J., 189, 441.
Monteiro, T.S., 1985, M.N.R.A.S. 214, 419.
Scharmer, G.B., Carlsson, M. 1985, Journal of Comp. Phys., 59, 56.
Schönberg, K., 1988, Astron. Astrophys., 195, 198.
Schönberg, K., Hempe, K., 1986, Astron. Astrophys., 163, 151.
Scoville, N.Z., Solomon, P.M., Ap. J. Letters, 187, L67.
Viscuso, P.J., Chernoff, D.F., 1988, Ap. J., 327, 364.
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 1989 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
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
Download citation
DOI: https://doi.org/10.1007/BFb0119506
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-51297-4
Online ISBN: 978-3-540-46187-6
eBook Packages: Springer Book Archive