William A. DentI am studying the variability of radio emission from quasars and active galactic nuclei at millimeter and centimeter wavelengths. This research program has two components: observational and interpretational.
Flux density measurements of over 100 known variable sources are made at regular intervals using the 120 ft. Haystack antenna, the 12-meter NRAO antenna on Kitt Peak and the 14-meter FCRAO antenna. Because the work needs a precision of 1%, careful attention must be paid to the pointing accuracy and gain calibration of the antenna. From these measurements which range in frequency from 7.8 GHz to 90 GHz, I can observe the time evolution of the synchrotron radiation spectrum. In many objects a series of outbursts with self-absorbed spectra and duration of a few years are seen along with more slowly varying components.
With an accumulated database of over 20 years, my collaborators and I are now attempting to understand this phenomena and answer the following questions about quasi-stellar radio sources: do the radio outbursts occur periodically; if so, why? How are the radio outbursts correlated with outbursts seen in the optical and X-ray bands? How are the outbursts related to structural changes observed with milliarc second resolution radio interferometer? What does the outburst profile tell us about particle acceleration and energy loss mechanisms occuring in the source? The answers to these questions may help us to understand the origin of the enormous amounts of energy being released in the nuclei of active galaxies.
dent@donald.phast.umass.edu
Last Update: 5/23/1993