Published May 1, 2017 | Version v1
Dataset Open

PARSEC V1.2S Core Overshooting Grid

Authors/Creators

  • 1. Harvard-Smithsonian Center for Astrophysics, NSF AAPF
  • 2. INAF Padova, Padova, Italy
  • 3. University of Washington
  • 4. University of California San Diego
  • 5. Raytheon Company
  • 6. SISSA, Trieste
  • 7. University of California Berkeley
  • 8. MPIA Heidelberg
  • 9. Space Telescope Science Institute

Description

Stellar evolution models calculated based on PARSEC V1.2S with a range of core overshooting strength. These models were used and  presented in Rosenfield et al., 2017, "A NEW APPROACH TO CONVECTIVE CORE OVERSHOOTING: PROBABILISTIC CONSTRAINTS FROM COLOR-MAGNITUDE DIAGRAMS OF LMC CLUSTERS"

Files

Files (90.8 MB)

Name Size Download all
md5:0f57cbf78b20a1bc45ea86d1667ac85e
90.8 MB Download