2 papers
astro-ph.SR2025
High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks
A. C. Rubio, A. C. Carciofi, J. E. Bjorkman +5
Binarity in massive stars has proven to be an important aspect in the their evolution. For Be stars, it might be the cause of their spin up, and thus part of the mechanism behind t…
astro-ph.SR2023
Modeling Variable Linear Polarization Produced by Co-Rotating Interaction Regions (CIRs) Across Optical Recombination Lines of Wolf-Rayet Stars
R Ignace, J E Bjorkman, A-N Chene +5
Massive star winds are structured both stochastically ("clumps") and often coherently (Co-rotation Interaction Regions, or CIRs). Evidence for CIRs threading the winds of Wolf-Raye…