Abstract
THE BINARY STAR ξ Booms.—Dr. Doberck, of the Markree Observatory, has published elements of this revolving doublestar, which appear to represent very satisfactorily the measures up to the present time, allowance being made for some obvious errors of observation. The orbit, which differs materially from those calculated upon shorter series of measures by Mädler, Herschel, and Hind, is as follows:—
Article PDF
Rights and permissions
About this article
Cite this article
Our Astronomical Column . Nature 15, 414 (1877). https://doi.org/10.1038/015414a0
Issue Date:
DOI: https://doi.org/10.1038/015414a0