AbstractAbstract
[en] IRAS 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)
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Source
National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center; vp; May 1987; vp; Star formation in galaxies; Pasadena, CA (USA); 16-19 Jun 1986; Available from NTIS, PC A99/MF E03
Record Type
Report
Literature Type
Conference; Numerical Data
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