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Infrared Imaging and Photometry of a Sample of Seyfert Galaxies

Published online by Cambridge University Press:  07 August 2017

V. Zitelli ,
R. Wade ,
L. Danese ,
G. De Zotti ,
G. Granato  and
N. Mandolesi
V. Zitelli
Affiliation:
Dip. di Astronomia, Via Zamboni 33, 40126 - Bologna - ITALY
R. Wade
Affiliation:
Royal Observatory, Blackford Hill - Edinburgh EH93HJ - SCOTLAND
L. Danese
Affiliation:
Dip. di Astronomia, Vicolo dell'Osservatorio 5, 35122 - Padova - ITALY
G. De Zotti
Affiliation:
Oss. Astronomico, Vicolo dell'Osservatorio 5, 35122 - Padova - ITALY
G. Granato
Affiliation:
Dip. di Astronomia, Vicolo dell'Osservatorio 5, 35122 - Padova - ITALY
N. Mandolesi
Affiliation:
ITESRE/CNR, Via Castagnoli 1,40126 - Bologna - ITALY

Extract

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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 

References

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