Computer Science
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phdt.........6b&link_type=abstract
Ph.D. Thesis Massachusetts Univ., Amherst.
Computer Science
41
Extragalactic Radio Sources, Flux Density, Stellar Evolution, Correlation, Radio Emission, Time Lag, Variability
Scientific paper
In order to investigate the evolution of compact extragalactic radio sources, three observing programs were undertaken. These programs were: single epoch spectra for 113 sources compiled from near simultaneous observations at seven frequencies (between 1.4 and 90 GHz); monthly observations were conducted at lambda 3 mm to search for short timescale variations; and radio (15.5 GHz) and optical variations in 45 sources were searched for correlated activity. The observed radio spectra are the first compilation of near simultaneous observations of this sample of regularly monitored variable sources. These sources exhibit a wide range of variability and spectral characteristics, thus constituting a useful sampler for comparison with theoretical models for radio emission mechanisms. The high frequency radio observations of varible extragalactic radio sources are important for studying the evolution of flux density outbursts, which are affected at lower frequencies by opacity effects and expansion processes.
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