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IRAS observations of BL Lac objectsIRAS data was analyzed for 35 BL Lac objects selected from a complete 5 GHz radio sample, using the coadded survey database. The detection rate is 50% with more than 40% detected in more than one band. This compares with only 15% of these sources that are included in the IRAS Point Source Catalog. High luminosity BL Lac objects generally have smooth energy spectra over four or five decades in frequency, consistent with incoherent synchrotron emission from 1 cm to 1 micron. However, many low luminosity BL Lac objects have discontinuous spectra, with a large range in the spectral index at IRAS wavelengths. For BL Lacs with a total luminosity of less than 10 to the 44th power ergs/-s, most of the far infrared energy probably originates from dust heated near the galaxy nucleus. The energy budget shows that the majority of the power per unit bandwidth emerges in the infrared (1 to 100 microns).
Document ID
19870014940
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Impey, C.
(California Inst. of Tech. Pasadena, CA, United States)
Neugebauer, G.
(California Inst. of Tech. Pasadena, CA, United States)
Miley, G.
(Space Telescope Science Inst. Baltimore, Md., United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington Star Formation in Galaxies
Subject Category
Astronomy
Accession Number
87N24373
Funding Number(s)
CONTRACT_GRANT: JPL-97582
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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