Abstract
“35 CAMELOPARDI,” B.A.C. 1924.—The principal component of this double star is not included either amongst the certain or suspected variables in Professor Schön-feld's last catalogue, but there would appear to be sufficient evidence of change to justify its being placed in the former class. Variability was suspected by the Baron Dembowski from his own estimates of magnitude 1865–68 (A.N. 1810), and the following are almost decisive of fluctuation through about two magnitudes, so that at times the star will be visible to the naked eye, and at others fairly beyond unassisted vision.
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Our Astronomical Column . Nature 12, 476–477 (1875). https://doi.org/10.1038/012476d0
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DOI: https://doi.org/10.1038/012476d0