The Young Planet DS Tuc Ab Has a Low Obliquity

@article{Montet2019TheYP,
  title={The Young Planet DS Tuc Ab Has a Low Obliquity},
  author={Benjamin T. Montet and Adina D. Feinstein and Rodrigo Luger and Megan Bedell and Michael A. Gully-Santiago and Johanna K. Teske and Sharon Xuesong Wang and R. Paul Butler and E. E. Flowers and Stephen A. Shectman and Jeffrey D. Crane and Ian B. Thompson},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2019}
}
The abundance of short-period planetary systems with high orbital obliquities relative to the spin of their host stars is often taken as evidence that scattering processes play important roles in the formation and evolution of these systems. More recent studies have suggested that wide binary companions can tilt protoplanetary disks, inducing a high stellar obliquity that form through smooth processes like disk migration. DS Tuc Ab, a transiting planet with an 8.138 day period in the 40 Myr… Expand

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