Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Positive Superhumps in High-mass-ratio Cataclysmic Variables Driven by Apsidal Disk Precession

  • Authors: Rebecca G. Martin, Stephen H. Lubow, David Vallet, Stephen Lepp

Rebecca G. Martin et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

Results of the SPH simulations. The disk eccentricity, longitude of periapsis, and total disk mass as a function of time at a radius of r = 0.6 rl for SPH simulations with q = 0.1 (top left), q = 0.2 (top right), q = 0.4 (bottom left), and q = 0.6 (bottom right).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse