Variability of the optical counterpart of OA 33

Details Variability of the optical counterpart of OA 33 Variability of the optical counterpart of OA 33

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90...24d&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Feb.-Mar. 1978, p. 24-27.

Astronomy and Astrophysics

Astronomy

3

Photographic Measurement, Radio Sources (Astronomy), Variable Stars, Visual Photometry, Astronomical Photometry, Quasars, Radio Spectra, Stellar Magnitude

Scientific paper

Optical and radio observations made near the flat-spectrum radio source OA 33 (5C3.50) have revealed a faint blue stellar object which shows evidence of variability of one magnitude in the 19m to 20m range. A Cuffey Iris Astrophotometer was used to determine magnitudes of both the object and comparison stars. Calibration curves are discussed for various photographic plates.

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