Models of Tidally Induced Gas Filaments in the Magellanic Stream
Authors: Stephen A. Pardy, Elena D'Onghia, and Andrew J. Fox
2018 The Astrophysical Journal857101.
Provider: AAS Journals
Caption: Figure 1.
Orbit of the SMC around the LMC in the model with a 9:1 mass ratio. The orbit before entering the MW potential is shown as a black solid line, and the orbit after entering it is shown with a red dashed line.