The energy of this process is given by a power law of temperature to the 19.9.
The energy of this process is given by a power law of temperature to the 19.9. The products of thisprocess are mixed in the second dredge-up. The cores of entities in the upper portion of the main sequenceis dominated by convection driven by this process. This process produces 26.8 MeV of energy, along with 3gamma rays, two positrons, and three electron neutrinos. This process becomes dominant at a temperatureof around 17 million kelvin and in stars greater than 1.3 (*) solar masses, and in this process, four protons fusetogether to form a helium atom. It is sometimes named for Bethe and Wiesczaker. Minor branches of this processcreate fluorine-18 and fluorine-19 along with its namesake elements. For 10 points, name this stellar nucleosynthesisreaction that dominates over the proton-proton chain in heavier stars, named for the three elements that comprise it.
The energy of this process is given by a power law of temperature to the 19.9.
CNO cycle [or carbon-nitrogen-oxygen cycle; prompt on stellar "nucleosynthesis" or "fusion"]