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Showing 1–4 of 4 results
Advanced filters: Author: Aldo M. Serenelli Clear advanced filters

  • Measurements of a precursor to a low-mass white-dwarf star reveal that such white-dwarf stars probably had a thick hydrogen envelope, which was lost by irradiation or shell flashes in the case of rapidly cooling white-dwarf stars.

    • Pierre F. L. Maxted
    • Aldo M. Serenelli
    • Veronika Schaffenroth
    Research
    Nature
    Volume: 498, P: 463-465

  • Bright star \(\nu\) Indi shows elevated levels of alpha-process elements, suggesting great age, and is kinematically heated, probably from the merger of a dwarf galaxy with the Milky Way. Chaplin et al. make a case for \(\nu\) Indi being an accurate indicator of the timing for the Gaia–Enceladus merger.

    • William J. Chaplin
    • Aldo M. Serenelli
    • Mutlu Yıldız
    Research
    Nature Astronomy
    Volume: 4, P: 382-389

  • All components of the proton–proton nuclear fusion chain, in which hydrogen is converted into helium in the Sun, are described, with several implications for fundamental solar and particle physics.

    • M. Agostini
    • K. Altenmüller
    • G. Zuzel
    Research
    Nature
    Volume: 562, P: 505-510