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ABSTRACT BINARY STARS.—From one of tlie very careful and complete investigations on the orbits of the revolving double stars, by which Dr. Doberck is so greatly contributing to our knowledge
of the motions of these interesting objects, we have an orbit of ɛ Scorpii which is probably a very near approximation to the true one. Access through your institution Buy or subscribe This
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THIS ARTICLE CITE THIS ARTICLE _Our Astronomical Column_ . _Nature_ 15, 500 (1877). https://doi.org/10.1038/015500a0 Download citation * Issue Date: 05 April 1877 * DOI:
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