SLOW SPIN CORES. “Asteroseismic data for low-mass stars have convincingly demonstrated that the cores of low-mass stars rotate at least an order of magnitude slower than predicted by most prior stellar models. Their predictions of compact object rotation rates are unreliable. We predict extremely slow rotation a ~ 10−2 for BHs born from single stars.” (BH = black hole).
https://lnkd.in/dApxk5K
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022