Classical Novae

Classical Novae is a cataclysmic variable star phenomenon characterized by a sudden, dramatic increase in luminosity due to thermonuclear runaway of accreted hydrogen on the surface of a white dwarf in a close binary system.

360

Publications

15.7K

Citations

667

Authors

397

Institutions

Publications per year

2017–2026

64

Authors

667

  1. SS
    S. Starrfield

    Arizona State University, United States

    22 publications · 1.3K citations

    20

    h-index

  2. MM
    Michael M. Shara

    American Museum of Natural History, United States

    24 publications · 1K citations

    18

    h-index

  3. MH
    M. Hernanz

    Institute of Space Sciences, Spain

    18 publications · 1.3K citations

    15

    h-index

  4. IH
    Izumi Hachisu

    The University of Tokyo, Japan

    13 publications · 770 citations

    13

    h-index

  5. BD
    Brian D. Metzger

    Columbia University, United States

    13 publications · 569 citations

    13

    h-index

1–5 of 667

Venues

  1. The Astrophysical Journal

    ApJ · 126 publications · 6.9K citations

    48

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    69 publications · 2.6K citations

    28

    h-index

  3. Astronomy and Astrophysics

    43 publications · 1.7K citations

    23

    h-index

  4. The Astronomical Journal

    AJ · 15 publications · 472 citations

    13

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 10 publications · 727 citations

    10

    h-index

1–5