Analysis of compact radio sources using 102 MHz interplanetary scintillation observations

Details Analysis of compact radio sources using 102 MHz interplanetary scintillation observations Analysis of compact radio sources using 102 MHz interplanetary scintillation observations

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997arep...41..723t&link_type=abstract

Astronomy Reports, Volume 41, Issue 6, November 1997, pp.723-733

Astronomy and Astrophysics

Astronomy

3

Scientific paper

An analysis of 125 radio sources from a 102 MHz survey of scintillating sources is presented. These compact (<1") radio sources are identified with radio sources in the most sensitive catalogs currently available. Analysis of the integrated spectra for these objects indicates that the compact sources have steep spectra (alpha > 0.5). There is a tendency for weaker sources to be more compact. The inferred spectral indices for compact sources in the cores of extended objects are on average lower than the integrated values. The most likely candidates for optical counterparts to the compact radio sources from the scintillating source survey are steep-spectrum quasars.

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