Nova Nucleosynthesis

Nova Nucleosynthesis is a theoretical framework in nuclear astrophysics that describes the rapid proton-capture processes and associated nuclear reaction networks occurring during explosive hydrogen burning in classical novae, distinguishing it from other stellar nucleosynthesis mechanisms by its specific thermonuclear runaway conditions on the surface of accreting white dwarfs.

178

Publications

9.8K

Citations

635

Authors

289

Institutions

Publications per year

2017–2026

25

Authors

635

  1. SS
    S. Starrfield

    Arizona State University, United States

    22 publications · 1.4K citations

    17

    h-index

  2. JJ
    J. José

    Universitat Politècnica de Catalunya, Spain

    17 publications · 1.6K citations

    16

    h-index

  3. MH
    M. Hernanz

    Institute of Space Sciences, Spain

    16 publications · 1.6K citations

    14

    h-index

  4. JW
    J. W. Truran

    University of Chicago, United States

    11 publications · 624 citations

    10

    h-index

  5. JW
    J. W. Truran

    University of Chicago, United States

    8 publications · 641 citations

    8

    h-index

1–5 of 635

Venues

  1. The Astrophysical Journal

    ApJ · 73 publications · 5.7K citations

    40

    h-index

  2. 13

    h-index

  3. Astronomy and Astrophysics

    12 publications · 491 citations

    12

    h-index

  4. Nature

    5 publications · 151 citations

    5

    h-index

  5. Nuclear Physics A

    5 publications · 211 citations

    5

    h-index

1–5