1 code implementation • 29 May 2019 • Sihao Cheng, Jeffrey D. Cummings, Brice Ménard
We show that, in addition to crystallization and merger delays, an $8$-Gyr cooling delay is required on the Q branch, which affects about $7\%$ of high-mass WDs.
Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
