Abstract
The information provided mostly by R. S. Harrington and by S. L. Lippincott is listed below in order of estimated mass of the companion upwards from 0.005 ℳ⊙ but not more than 0.5 ℳ⊙. For each star are given the position referring to the equator, equinox and epoch of the year 2000, the apparent visual magnitude, spectrum, parallax as well as the period of revolution P, eccentricity e of the perturbation orbit and the adopted value for the mass M B of the unseen companion (Chapter 11, formulae (11.17ff)). Only for two stars, Ross 614 and VW Cephei the companion has been seen later (Chapter 14).
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© 1986 D. Reidel Publishing Company
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Van De Kamp, P. (1986). Perturbations. Current Photographic Studies. In: Dark Companions of Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4692-7_14
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DOI: https://doi.org/10.1007/978-94-009-4692-7_14
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8586-1
Online ISBN: 978-94-009-4692-7
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