Possible Secular Variation of the Flux and Spectrum of Radio Emissions of Source 1934-63

Details Possible Secular Variation of the Flux and Spectrum of Radio Emissions of Source 1934-63 Possible Secular Variation of the Flux and Spectrum of Radio Emissions of Source 1934-63

Apr 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965natur.206..176s&link_type=abstract

Nature, Volume 206, Issue 4980, pp. 176-177 (1965).

Physics

28

Scientific paper

THE recently studied source 1934-631 is characterized by maximum spectral flux density at a frequency of νm ~= 600 Mc/s. Recently, spectra of this type have been obtained for a number of sources, some of which are identified with quasi-stellar objects (for example, 3C-48). In none of the known sources of this type, however, does the frequency of the maximum reach such a high value as in the case of 1934-63.

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