Abstract
The masses of double-lined photometric pairs can be found directly from the orbit, as was mentioned earlier. Almost all of the systems selected in Table III have this qualification that good photometric orbits are supplemented by radial-velocity solutions from double-lined spectra.
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© 1978 D. Reidel Publishing Company, Dordrecht, Holland
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Heintz, W.D. (1978). Mass Determinations From the MLR. In: Double Stars. Geophysics and Astrophysics Monographs, vol 15. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9836-0_43
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DOI: https://doi.org/10.1007/978-94-009-9836-0_43
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-0886-1
Online ISBN: 978-94-009-9836-0
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