Image Details

Choose export citation format:

The YREC Stellar Evolution Code: Public Data Release

  • Authors: Marc H. Pinsonneault, Jennifer L. van Saders, Lyra Cao, Jamie Tayar, Franck Delahaye, Leslie M. Morales, Rachel A. Patton, Matthew C. Rendina, Joel C. Zinn, Zachary R. Claytor, Amanda L. Ash, Susan Byrom, Kaili Cao, Vincent A. Smedile

Marc H. Pinsonneault et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 18.

Radial rotation profiles for a 3 M star halfway through helium burning. Convective regions are pink in all cases. We enforce various rotation profiles, including solid body for the whole star (blue), a solid-body interior and a differentially rotating surface convection zone (green), and solid-body convection zones but a differentially rotating radiative region (orange).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse