Photoelectric observations of a magnitude and color variable object in Perseus

Details Photoelectric observations of a magnitude and color variable object in Perseus Photoelectric observations of a magnitude and color variable object in Perseus

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..252c&link_type=abstract

(Acta Astronomica Sinica, vol. 21, Sept. 1980, p. 252-256.) Chinese Astronomy and Astrophysics, vol. 5, June 1981, p. 152-156. T

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, B Stars, Early Stars, Electrophotometers, Light Curve, Ubv Spectra, Color, Periodic Variations, Radiant Flux Density, Shell Stars, Stellar Envelopes, Stellar Magnitude

Scientific paper

U(prime), B(prime), and V(prime) photoelectric observations are made of the light and color variable object (radio N-galaxy) in Perseus. The object is found to differ from the typical early type shell star BU Tau in two respects. One is that its amplitude in U(prime) is greater than that in B(prime); the second is that its U(prime) magnitude is positively correlated with U(prime) - B(prime and uncorrelated with B(prime) - V(prime).

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