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Infrared-Selected “Warm” Galaxies Observed in X-rays
Published online by Cambridge University Press: 07 August 2017
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The Infrared Astronomical Satellite (IRAS) has detected many galaxies in the infrared (IR), most of which have fairly steep 25μ to 60μ spectra. Many quasars and active galaxies exhibit a significantly flatter spectrum in the infrared. Several studies, for example, DeGrijp et al. (1985) used this characteristic to select a subsample of “warm” objects from the IRAS PSC (1985).
- Type
- Part 7: Dust, Molecules, Infrared and MM Radiation
- Information
- Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 420 - 421
- Copyright
- Copyright © Kluwer 1989
References
IRAS Catalogs and Atlases: Point Source Catalog
1985 (Washington, D. C.: U. S. Government Printing Office).Google Scholar
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