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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 2.

The disk surface density (upper) and eccentricity (lower) as a function of radius at a time of t = 50 Pb (left) and t = 100 Pb (right) for the SPH simulations.

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