In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 134 ( 1989), p. 49-50
Abstract:
We have observed a homogeneous sample of Seyfert 1 and 1.5 galaxies with the aim to determine the luminosity function of Seyfert nuclei. Observations were made with the CCD cameras of Asiago and Loiano Observatories in B, V and R bands in order to isolate the contribution of different stellar populations. A photometric decomposition into three components (disc, bulge and nucleus) was fitted to the observed luminosity profiles to separate the nuclear and the host galaxy contributions and to understand whether underlying galaxies actually behave as “normal” galaxies.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900140331
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1989
SSG:
16,12