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318-MHz variability of complete samples of extragalactic radio sources

Journal Article · · Astron. J.; (United States)
DOI:https://doi.org/10.1086/112381· OSTI ID:6799162
Flux-density measurements at 318 MHz were made during two epochs, separated by approximately 7 yr, of extragalactic sources in samples complete to 3 Jy at 1400 MHz and 1 Jy at 5000 MHz. Steep-spectrum (..cap alpha..> or =+0.5) sources do not appear to vary, but at least 1/4 of the flat-spectrum (..cap alpha..<+0.5) sources observed were found to be low-frequency variables on time scales of decades. Several 318 and 606 MHz flux-density measurements made from 1969 to 1971 confirm Hunstead's discovery (Astrophys. Lett. 12, 193 (1972)) of 408-MHz variability in 3C 454.3 on a time scale of only a few years. Various explanations for low-frequency variability: noncosmological redshifts, intergalactic scintillations, variable absorbing shells, coherent emission mechanisms, special geometries, and relativistic expansion of incoherent electron--synchrotron components: were considered in the light of the observations. We conclude that relativistic expansion of sources emitting incoherent electron--synchrotron radiation is in best agreement with the data, although the rapid variations observed in 3C 454.3 during 1969--1971 are still difficult to understand quantitatively.
Research Organization:
National Radio Astronomy Observatory, Edgemont Road, Charlottesville, Virginia 22901
OSTI ID:
6799162
Journal Information:
Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 84:1; ISSN ANJOA
Country of Publication:
United States
Language:
English