Star formation in Seyfert galaxies

Bibcode
1987NASCP2466..669E
Rodriguez Espinosa, J. M.; Rudy, Richard J.; Jones, Barbara
Referencia bibliográfica

In NASA, Washington Star Formation in Galaxies p 669-674 (SEE N87-24266 17-89)

Fecha de publicación:
5
1987
Número de autores
3
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro
Galaxias Seyfert
Formación estelar
Astronomía infrarroja
Galaxias espirales
Galaxias con estallidos

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