Abstract
Several recent observational determinations of the distribution of separations of wide binaries are critically reviewed and compared with the distributions inferred from observational work on pre-main sequence stars and from theoretical ideas on binary formation. It is concluded that it is not very fruitful to depict the whole distribution function of separations by one law, and that it is preferable to represent separately the two main mechanisms of binary formation, namely first-collapse fragmentation (for s > 25 AU) and disk fragmentation (for s < 25 AU). It is also found that the best representation for the group of wide binaries (s > 25 AU) is given by Öpik’s law ρ(s) = ks -2, but that this distribution has a cutoff that is age-dependent. This cutoff is interpreted in terms of the dynamical evolution of wide binaries.
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© 1997 Kluwer Academic Publishers
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Allen, C., Poveda, A., Herrera, M.A. (1997). The Distribution of Separations of Wide Binaries. In: Docobo, J.A., Elipe, A., McAlister, H. (eds) Visual Double Stars: Formation, Dynamics and Evolutionary Tracks. Astrophysics and Space Science Library, vol 223. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1477-3_18
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DOI: https://doi.org/10.1007/978-94-009-1477-3_18
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