Bibcode
Rodriguez Espinosa, J. M.; Rudy, Richard J.; Jones, Barbara
Bibliographical reference
In NASA, Washington Star Formation in Galaxies p 669-674 (SEE N87-24266 17-89)
Advertised on:
5
1987
Citations
0
Refereed citations
0
Description
An analysis of the IRAS data for a sample of classical (optically
selected) Seyfert galaxies is presented. The IRAS fluxes at 25 micron,
60 micron, and 100 micron are found to be uncorrelated or only very
weakly correlated with the UV/Optical continuum flux and the near and
mid IR flux at 3.5 and 10 microns. To investigate the possibility that
star formation accounts for the far IR flux, the IRAS measurements for
the Seyfert galaxies are compared to IRAS observations of a sample of
normal spiral galaxies, and a sample of Starburst galaxies. It is shown
that the far IR luminosities and far IR colors of Seyfert galaxies are
indistinguishable from those of the Starburst galaxies. Besides, normal
galaxies are an order of magnitude less luminous than both the Seyfert
and the Starburst galaxies. This indicates that star formation produces
the bulk of the far infrared emission in Seyfert galaxies.