Abstract
Spectral measurements of the two BL Lac objects OQ 530 and ON 325 are
presented. The measurements were taken at frequencies ranging from radio
to ultraviolet. Both sources show spectral curvature between the
infrared and ultraviolet frequencies. The intensity and spectral shape
of OQ 530 vary, but the spectral shape of ON 325 appears to remain
constant during intensity variability. A nonthermal theoretical model of
jet emission is developed which incorporates both the spectral and time
variability data. The model predicts that ON 325 radiates at X-ray
frequencies with Compton radiation dominating over synchrotron emission.
The angular size of the jet emission is predicted to be less than 0.1
milli-arcsec at high radio frequencies.
Original language | English |
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Pages (from-to) | 512-518 |
Journal | Astrophysical Journal |
Volume | 284 |
Publication status | Published - 1 Sept 1984 |
Keywords
- Astronomical Spectroscopy
- Bl Lacertae Objects
- Radiation Sources
- Compton Effect
- Infrared Spectra
- Iue
- Radio Spectra
- Synchrotron Radiation
- X Ray Spectra