Correlation between the optical and time-delayed radio variability of the NGC 1275 radio source

Details Correlation between the optical and time-delayed radio variability of the NGC 1275 radio source Correlation between the optical and time-delayed radio variability of the NGC 1275 radio source

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..223l&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Apr. 1980, p. 223-226.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 122-124

Astronomy and Astrophysics

Astronomy

7

Extragalactic Radio Sources, Light Curve, Periodic Variations, Electrophotometry, Time Lag

Scientific paper

Comparison of the radio and optical variability of the extragalactic
radio source NGC 1275 (Perseus A) for 1966-1978 shows that the optical
variability is 2.2 yr ahead of the slow radio component at 1-10 mm
wavelength and 5.5 yr ahead at 2.8 cm wavelength. These radio delays
suggest that the optical and radio emission come from different regions.

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