Excess 2 centimeter emission - a new continuum component in the spectra of radio-quiet quasars
The centimeter and millimeter regions of the spectra of radio-quiet quasars and luminous Seyfert 1 nuclei are examined. It is found that steep-spectrum optically thin synchrotron radiation dominates in the 20 cm to 6 cm region of most objects. A flat or rising component which becomes dominant by 2 cm in nine of the 17 cases in the sample is identified as a new continuum component called the high-frequency excess (HFE). The luminous quasar PG 1634 + 706, for which HFE dominates throughout the centimeter region, is discussed in detail. Possible causes of the HFE include self-absorbed synchrotron sources, about 10 to the 6 K nuclear free-free sources, and about 1000 K free-free sources from associated nuclear starbursts. It is concluded that because the brightness temperature predictions are very distinct, future observations will determine which explanation is correct. 27 references.
- Research Organization:
- Space Telescope Science Institute, Baltimore, MD (USA); National Radio Astronomy Observatory, Charlottesville, VA (USA); Haystack Observatory, Westford, MA (USA)
- OSTI ID:
- 6685096
- Journal Information:
- Astrophys. J.; (United States), Vol. 332
- Country of Publication:
- United States
- Language:
- English
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