no code implementations • 9 Mar 2021 • J. X. Luu, D. C. Jewitt, M. Mutchler, J. Agarwal, Y. Kim, J. Li, H. Weaver
The character of the emission, including its episodic nature and the low speed of the ejected particles ($V \sim $ 0. 15 m s$^{-1}$), is most consistent with mass loss from a body rotating near rotational breakup.
Earth and Planetary Astrophysics
