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Line 57: == Eccentric orbit == In an orbit with eccentricity <math>e</math>, the mass function is given by<ref name="tauris" /><ref name="boffin">{{cite book \|last1=Boffin \|first1=H. M. J. \|editor1-last=Arenou \|editor1-first=F. \|editor2-last=Hestroffer \|editor2-first=D. \|title=Proceedings of the workshop "Orbital Couples: Pas de Deux in the Solar System and the Milky Way" ~~\|journal=Orbital Couples: Pas de Deux in the Solar System and the Milky Way~~ \|date=2012 \|pages=41–44 \|chapter=The mass-ratio distribution of spectroscopic binaries \|isbn=978-2-910015-64-0 \|name-list-style=amp\|bibcode=2012ocpd.conf...41B }}</ref> <math display="block">f = \frac{M_2^3 \sin^3 i }{(M_1 + M_2)^2} = \frac{P_\mathrm{orb}\ K^3}{2 \pi G} \left(1 - e^2\right)^{3/2}.</math>

Binary mass function: Difference between revisions