2004/12/15 by Daniele Galli, Galli, Daniele
Physics and Astronomy · #Astro and Planetary Science #Astrophysics (astro-ph) #Cosmology and Gravitation Theories #FOS: Physical sciences #Quantum, superfluid, helium dynamics #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0412380
6 pages, 2 figures. Invited talk presented at the ESO-ARCETRI workshop on "Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites" (September 13-17 2004), to be published in "ESO Astrophysics Symposia", Editors: L. Pasquini and S. Randich
arxiv created 2004/12/15 · openalex publication_date 2004/12/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We recall the emergence of the ``3He problem'', its currently accepted solution, and we summarize the presently available constraints on models of stellar nucleosynthesis and studies of Galactic chemical evolution from measurements of the abundance of 3He in the Galaxy.