Figure 7 from Models of Tidally Induced Gas Filaments in the Magellanic Stream

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Models of Tidally Induced Gas Filaments in the Magellanic Stream

Authors: Stephen A. Pardy, Elena D'Onghia, and Andrew J. Fox

2018 The Astrophysical Journal 857 101.

Provider: AAS Journals

Caption: Figure 7.

Representation in Magellanic Stream coordinates for interactions with different mass ratios. Each panel shows the density of gas in the simulations as in panel C of Figure 3.

Other Images in This Article

Copyright and Terms & Conditions