Fig. 4 from Branch, Spur, and Feather Formation in Spiral Galaxies

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Branch, Spur, and Feather Formation in Spiral Galaxies

Authors: S. Chakrabarti, G. Laughlin, and F. H. Shu

Chakrabarti, Laughlin, & Shu 2003 The Astrophysical Journal 596 220.

Provider: AAS Journals

Caption: Fig. 4.

(a) Response of the gas disk upon applying a transient leading spiral perturbation in the ﹩Q_{g}=1.3﹩ disk. Times are given in machine units (at ﹩\xi =1﹩, one full revolution requires ﹩t=39.2﹩). (b) Response of the gas disk upon applying a transient leading spiral perturbation in the ﹩Q_{g}=2.48﹩ disk.

Other Images in This Article

Copyright and Terms & Conditions