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39 ta ish

Ish: Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> synthesis and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> radiative capture

  1. The 12C(a,g)16O Cross Section at Low Energies

    F. C. Barker, T. Kajino

    Maqola199112 iqtibos
    ABI
  2. Sarlavhasiz

    Boshqa9 iqtibos
    ABI
  3. The 12C(α, γ)16O cross section at stellar energies

    A. Redder, Harry Becker, C. Rolfs +5

    Maqola19874 iqtibos
    ABI
  4. Energy levels of light nuclei A = 16–17

    D. R. Tilley, H. R. Weller, C. M. Cheves

    Maqola19932 iqtibos
    ABI