NDLI: Star formation in seyfert galaxies

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Star formation in seyfert galaxies

Content Provider	NASA Technical Reports Server (NTRS)
Author	Espinosa, J. M. Rodriguez Rudy, Richard J. Jones, Barbara
Copyright Year	1987
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.
File Size	348077
Page Count	6
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19870014931
Archival Resource Key	ark:/13960/t82k1b437
Language	English
Publisher Date	1987-05-01
Access Restriction	Open
Subject Keyword	Astrophysics Far Infrared Radiation Seyfert Galaxies Stellar Color Star Formation Starburst Galaxies Spectral Emission Infrared Astronomy Infrared Astronomy Satellite Spiral Galaxies Infrared Spectra Stellar Luminosity Galactic Nuclei Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Article

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