Research news on Stellar nucleosynthesis

Stellar nucleosynthesis is the research area concerned with the nuclear processes by which chemical elements are formed and transformed within stars and related astrophysical environments. It encompasses hydrogen burning (pp-chains, CNO cycles), helium burning, advanced hydrostatic burning stages (carbon, neon, oxygen, silicon burning), and explosive nucleosynthesis in supernovae and neutron-star-related events. The field integrates nuclear reaction theory and measurements, stellar structure and evolution modeling, and observational constraints from stellar spectra and isotopic abundances. A central focus is quantifying reaction rates and yields to explain the origin and distribution of isotopes in the cosmos and to constrain models of stellar evolution and galactic chemical evolution.

Forget stardust—it was star ice all along

Carl Sagan famously said that "We're all made of star stuff." But he didn't elaborate on how that actually happened. Yes, many of the molecules in our bodies could only have been created in massive supernovae explosions—hence ...

Want to find more supernovae? Follow the light

Is there anything more dramatic than an exploding star? More than just extraordinarily bright, energetic events that can light up the sky for months, these explosions play important roles in the cosmos. Supernovas create ...

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