Abstract
The 60 to 25 µm flux ratio of type 2 Seyferts is correlated with their emission line reddening in a way which is not consistent with a distributed heating source but agrees with predictions of a centrally heated dust shell model with a luminous UV power source.
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© 1988 Springer-Verlag
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Kailey, W.F., Lebofsky, M.J. (1988). Far infrared emission of type 2 seyferts. In: Lawrence, A. (eds) Comets to Cosmology. Lecture Notes in Physics, vol 297. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0118815
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DOI: https://doi.org/10.1007/BFb0118815
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