Linked from

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

• Eta CarinaeRelated: Material expelled by Eta Carinae carries products of nuclear processing into its surroundings.

• 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.

• Population II starRelated: Earlier stellar nucleosynthesis supplied the heavier elements in Population II birth clouds.

• Blue supergiantRelated: Fusion supplies the energy that sustains the star’s luminosity.

• Presolar grainRelated: Grain isotope ratios provide direct samples of stellar nucleosynthesis products.

• 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.

• Alpher–Bethe–Gamow paperCompared with: Later work showed that stars, not early-universe neutron capture alone, make most elements beyond helium.

• Carbon-based lifeRelated: Stellar processes created the carbon later incorporated into planets and living matter.

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

• Stellar astronomyRelated: Fusion inside stars powers them and builds many of the elements they later disperse.

• SupergiantRelated: Advanced fusion stages in massive supergiants build elements beyond those made by ordinary hydrogen burning.

• Universe (cosmology)Related: Most elements beyond the lightest primordial nuclei arose through processes in cosmic generations of stars.

• Allan SandageRelated: Nuclear-fuel models underpin the stellar-evolution calculations used to infer cluster ages.

• Big HistoryRelated: It explains how stars produced the elements needed for planets and life.

• 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.

• Composition of astronomical objectsRelated: Stellar abundance patterns record the nuclear processes that produced heavier elements.

• CW LeonisRelated: Dredged-up carbon connects the star’s composition to element production in evolved stars.

• Edwin E. SalpeterRelated: Salpeter calculated how nuclear reactions in stars build heavier elements.

• Formation and evolution of stars and galaxiesRelated: Stars produce and disperse many of the elements that later enrich galaxies.

• HypernovaRelated: Explosive burning during a hypernova can synthesize and disperse heavy elements.

• List of interstellar and circumstellar moleculesRelated: Circumstellar molecules can carry elements processed and expelled by stars.

• NGC 7027Related: The nebula's enriched gas records elements processed in its progenitor star.

• Timeline of the far futureRelated: The dwindling supply of star-forming gas helps explain why future star formation will decline.