Abstract
Binaries are not always neatly aligned. Previous observations of the DI Herculis system showed that the spin axes of both stars are highly inclined with respect to one another and the orbital axis. Here, we report on our ongoing survey to measure relative orientations of spin-axes in a number of eclipsing binary systems. These observations will hopefully lead to new insights into star and planet formation, as different formation scenarios predict different degrees of alignment and different dependencies on the system parameters. Measurements of spin-orbit angles in close binary systems will also create a basis for comparison for similar measurements involving close-in planets. © International Astronomical Union 2012.
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CITATION STYLE
Albrecht, S., Winn, J. N., Fabrycky, D. C., Torres, G., & Setiawan, J. (2011). The BANANA survey: Spin-orbit alignment in binary stars. In Proceedings of the International Astronomical Union (Vol. 7, pp. 397–398). Cambridge University Press. https://doi.org/10.1017/S1743921311027906
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