The Fine Structure of Cygnus A

Details The Fine Structure of Cygnus A The Fine Structure of Cygnus A

Mar 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971apl.....8...11m&link_type=abstract

Astrophysical Letters, Vol. 8, p.11-15

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

Results of the interferometric observations of Cygnus A at 2695 MHz with baselines of up to 3x105 wavelengths are presented. The two small radio cores have been resolved. The data for the westerly core can be explained by a double model with components extended by ~1 arc sec and separated by 4.6 arc sec in a position angle of 130 arc deg. The easterly core also consists of at least two components with sizes ~0.5-0.6 arc sec. Some astrophysical implications of this result are discussed.

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