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5 та иш

Иш: The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status

  1. Photonuclear reactions on stable isotopes of selenium at bremsstrahlung end-point energies of 10−23 MeV

    F. A. Rasulova, N. V. Aksenov, S.I. Alekseev +8

    МақолаNuclear physics research studiesChinese Physics C20230 иқтибос
    ABI

  2. Photonuclear reactions on stable isotopes of molybdenum at bremsstrahlung endpoint energies of 10–23 MeV

    F. A. Rasulova, N. V. Aksenov, Sergey Alekseev +6

    МақолаNuclear Physics and ApplicationsPhysical review. C20250 иқтибос
    ABI

  3. Low-energy upbend in the photon strength function of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Fe</mml:mi><mml:mprescripts/><mml:none/><mml:mn>57</mml:mn></mml:mmultiscripts></mml:math>

    Jan Kopecký, I. Tomandl

    МақолаNuclear physics research studiesPhysical review. C20250 иқтибос
    ABI

  4. Study of the reaction rates and cross sections of photonuclear reactions in natMg, natFe, and natNi nuclei at energies of up to 20 MeV

    E. T. Ruziev, Д. Л. Демин, S. A. Evseev +9

    МақолаRadiopharmaceutical Chemistry and ApplicationsThe European Physical Journal Plus20250 иқтибос
    ABI

  5. Molybdenum and ruthenium in the Galactic disk: A closer look at their nucleosynthesis components

    T. Mishenina, T. Kurtukian-Nieto, T. Gorbaneva +3

    МақолаStellar, planetary, and galactic studiesAstronomy and Astrophysics20250 иқтибос
    ABI