Abstract
We discuss the respective contributions of the interstellar radiation field and embedded stars to the heating of dust in molecular clouds, and present results of a comparison between far-IR and CO emission from nearby molecular clouds.
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References
Boulanger, F., and Pérault, M., 1988, Ap. J. in press.
Boulanger, F., Cohen, R.S., Gaida, M., Grenier, I., Koprucu, M., Maddalena, R.J., Thaddeus, P., and Ungerechts, H. 1988, in preparation
Dame, T.M., Ungerechts, R.S., Cohen, R.S., E. de Geus, Grenier, I.A., May, J., Murphy, D.C., Nyman, L.A., and Thaddeus, P. 1987, Ap. J., 322, 706
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© 1988 Springer-Verlag
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Boulanger, F. (1988). Comparison of Far-IR and CO emission from nearby molecular clouds. In: Dickman, R.L., Snell, R.L., Young, J.S. (eds) Molecular Clouds in the Milky Way and External Galaxies. Lecture Notes in Physics, vol 315. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-50438-9_238
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DOI: https://doi.org/10.1007/3-540-50438-9_238
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