Linked from

The 78 pages that link to Stellar nucleosynthesis, each with the reason it gives.

• MetallicityNarrower topic: Stellar fusion and subsequent burning stages produce many elements that raise metallicity.

• SupernovaNarrower topic: Explosive reactions forge and disperse many elements heavier than iron.

• LithiumNarrower topic: Stellar processes both produce and destroy lithium, shaping its cosmic abundance.

• Red giantNarrower topic: Red-giant fusion builds some heavier elements and alters the star’s composition.

• CarbonNarrower topic: Carbon’s cosmic abundance emerges from the broader history of element formation.

• Supernova nucleosynthesisNarrower topic: Supernova nucleosynthesis extends element production beyond the star's pre-explosion burning stages.

• Helium-4Narrower topic: Stars create helium-4 through hydrogen fusion and later nuclear burning.

• Triple-alpha processNarrower topic: This reaction is a central pathway by which stellar nucleosynthesis makes carbon.

• CNO cycleNarrower topic: The CNO cycle processes hydrogen and changes the isotope inventory inside stars.

• Margaret BurbidgeNarrower topic: This broader subject encompasses the element-making processes clarified in Burbidge's work.

• Red supergiantNarrower topic: A red supergiant builds heavier nuclei in its core and surrounding shells.

• S-processNarrower topic: The s-process is one pathway by which stars synthesize elements heavier than iron.

• B2FH paperNarrower topic: The paper organized the known processes of element formation inside stars.

• Helium burningNarrower topic: Helium burning is one stage in the larger sequence of element-making reactions in stars.

• Helium flashNarrower topic: The flash initiates core fusion that builds carbon and oxygen from helium.

• Geoffrey BurbidgeNarrower topic: It is the central research area to which Burbidge made lasting theoretical and observational contributions.

• Pair-instability supernovaNarrower topic: The explosion synthesizes and ejects large quantities of elements, including radioactive nickel.

• Stellar coreNarrower topic: Successive core-burning stages build elements beyond the helium made during hydrogen fusion.

• Solar coreNarrower topic: Core fusion is the Sun’s present-day contribution to this broader process.

• William Alfred FowlerNarrower topic: It is the central astrophysical process Fowler’s research helped quantify.

• Isotopes of oxygenNarrower topic: Stellar reactions forge oxygen nuclei, including the abundant oxygen-16 isotope.

• Carbon burningNarrower topic: Carbon burning is one stage in the sequence that builds elements inside stars.

• Local BubbleNarrower topic: Supernovae associated with the Bubble's history also enriched nearby space with newly made elements.

• Chemically peculiar starNarrower topic: Some surface anomalies reflect material processed by nuclear reactions and brought upward.