Oscillatory Model for Radio Source 3C273

Details Oscillatory Model for Radio Source 3C273 Oscillatory Model for Radio Source 3C273

Mar 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.201q1016a&link_type=abstract

Nature, Volume 201, Issue 4923, pp. 1016 (1964).

Physics

Scientific paper

THE radio source 3C273 has recently been identified with a star-like, superluminous object of thirteenth apparent magnitude1,2. Doppler shift measurements of identifiable line features indicate a strong red shift corresponding to radial velocity of 4 × 109 cm/sec, while the observed spectral characteristics of the continuum suggests synchrotron radiation as the dominant emission mechanism3.

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