Image Details
Caption: Fig. 3.
Summary of the results of the spectral classification as a function of the infrared luminosity. The results from the present paper were combined with those obtained by Veilleux et al. (1995) on LIGs in the BGS. The fraction of Seyfert galaxies increases with infrared luminosity.
© 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.