IRAS Observations of Active Galaxies
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert galaxies occupy much the same area in color-color plots as do normal infrared bright galaxies, but extend the range towards flatter 60–25 µm slopes. Statistically the Seyfert 1 galaxies can be distinguished from the Seyfert 2 galaxies, lying predominantly closer to the area with constant slopes between 25 and 100 µm. The infrared measurements of the Seyfert galaxies cannot distinguish between the emission mechanisms in these objects although they agree with the currently popular ideas; they do provide a measure of the total luminosity of the Seyferts. The quasar’s position in the color-color diagrams continue the trend of the Seyferts. The quasar 3C48 is shown to be exceptional among the radio loud quasars in that it has a high infrared luminosity which dominates the power output of the quasar and is most likely associated with the underlying host galaxy.
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- Bregman, J. et al., 1985, Ap. J., submitted.Google Scholar
- The Explanatory Supplement to the IRAS Catalogs and Atlases 1985, edited by Beichman, C.A., Neugebauer, G., Habing, H.J., Clegg, P.E., and Chester, T.J. (Washington D.C., U.S. Government Printing Office).Google Scholar
- deGrijp, M.H.K., Miley, G.K., Lub, J., deJong, T., 1985, Nature, in pressGoogle Scholar
- Fried, J. 1986, this volumeGoogle Scholar
- Helou, G. 1985, in preparationGoogle Scholar
- Miley, G.K., Neugebauer, G., and Soifer, B.T. 1985 Ap. J. (Letters), in press.Google Scholar
- Neugebauer, G., and Soifer, B.T. 1985, Ap.J. (Letters), submitted.Google Scholar
- Soifer, B.T. et al. 1985, in preparation.Google Scholar
- Veron-Cetty, M.P. and Veron, P. 1984, A Catalogue of Quasars and Active Nuclei, (Munich: European Southern Observatory).Google Scholar