The variability of the optical counterparts of four extragalactic radio sources

Details The variability of the optical counterparts of four extragalactic radio sources The variability of the optical counterparts of four extragalactic radio sources

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...52..289m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 52, May 1983, p. 289-291. Research supported by the Georgia

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Extragalactic Radio Sources, Light Curve, Calibrating, Data Reduction

Scientific paper

The optical variability of four extragalactic radio sources has been studied using the archival plates at the Harvard College Observatory. Three of these sources, PKS 1123 + 264, B2 1132 + 303, and 4C 18.36, were conclusively found to exhibit significant optical variability. No conclusive evidence was found for optical variability for B2 1128 + 315 with a range of less than 0.3 magnitude,, based on a limited number of plates.

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