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Infrared Imaging and Photometry of a Sample of Seyfert Galaxies
Published online by Cambridge University Press: 07 August 2017
Extract
It is well know that the determination of the local luminosity function of Seyfert nuclei meets several difficulties produced by: the determination of a suitable sample, the estimation of the nuclear magnitudes biased from the contribution from the host galaxies, which may be dominant if the nucleus is faints and the presumably large errors associated with the estimated magnitudes.
- Type
- Part 7: Dust, Molecules, Infrared and MM Radiation
- Information
- Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 412 - 413
- Copyright
- Copyright © Kluwer 1989