no code implementations • 15 Feb 2021 • Maria Hjorth, Simon Albrecht, Teruyuki Hirano, Joshua N. Winn, Rebekah I. Dawson, J. J. Zanazzi, Emil Knudstrup, Bun'ei Sato
In theory, star/disk misalignments can result from turbulence during star formation or the gravitational torque of a wide-orbiting companion star, but no definite examples of this scenario are known.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
