Physics of Eclipsing Binaries. III. Spin-Orbit Misalignment
Abstract
Binary systems where the axis of rotation (spin) of one or both components is tilted w.r.t. the axis of revolution are called misaligned binary systems. The angle of misalignment, obliquity, has been measured for a handful of stars and extrasolar planets to date. Here we present a mathematical framework for a complete and rigorous treatment of misalignment and introduce an extension to the public PHOEBE code that implements this framework. We discuss misalignment for the Roche geometry and introduce methods for computing stellar shapes, equilibrium (generalized Lagrange) points of the potential and minimal requirements for lobe existence. Efficient parametrization of misalignment is proposed in the plane-of-sky coordinates and implementation details in PHOEBE are given alongside the proof-of-concept toy model, comparison with a known misaligned binary DI Her, and comparison with a misaligned planetary system Kepler-13. We provide important mathematical details of the model in the Appendix. This paper accompanies the release of PHOEBE 2.1, which will be available soon from its website http://phoebe-project.org.
Keywords
Cite
@article{arxiv.1806.07680,
title = {Physics of Eclipsing Binaries. III. Spin-Orbit Misalignment},
author = {Martin Horvat and Kyle E. Conroy and Herbert Pablo and Kelly M. Hambleton and Angela Kochoska and Joseph Giammarco and Andrej Prša},
journal= {arXiv preprint arXiv:1806.07680},
year = {2019}
}
Comments
20 pages, 10 figures, published in ApJS; release of PHOEBE 2.1 is available at http://phoebe-project.org