The additional pressure raises the core temperature, andeventually it gets hot enough for the helium debris left over from themain sequence to begin f...sing into carbon and oxygen. This generatesenough heat to once again balance the gravitational pressure, and astate of equilibrium is regained.Eventually, the helium gets used up, and what happens next depends onthe star's mass. For stars like our sun, that's about it. It'll shrinkdown to a white dwarf star, shining feebly for a few million years. I have a feeling I’m going to be having more time to spend on some kind of project, now that my rehab is on track. Her next screen play is just the first of those projects. If it’s like the last one, it will make me crazy, but it will keep my mind active,” I explained.“Yeah, Yeah, you just like having a younger woman fawning all over you,” she said.“I like having you around sure, but none of you fawn,” I contradicted her.“Right,” she said. “Well you might be seeing more of me. She emailed. More

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