Pre-explosion Variability

Pre-Explosion Variability is an observational astrophysical phenomenon characterized by detectable fluctuations in the photometric, spectroscopic, or circumstellar properties of a massive star in the months to years immediately preceding its core-collapse or thermonuclear supernova explosion, distinguishing it from stable stellar evolution by signaling late-stage instabilities, mass-loss episodes, or binary interactions directly linked to the progenitor's impending disruption.

113

Publications

8.8K

Citations

777

Authors

316

Institutions

Publications per year

2017–2026

48

Authors

777

  1. AG
    A. Gal‐Yam

    Weizmann Institute of Science, Israel

    15 publications · 2.2K citations

    15

    h-index

  2. PN
    P. Nugent

    Lawrence Berkeley National Laboratory, United States

    12 publications · 1.9K citations

    12

    h-index

  3. DA
    D. A. Howell

    Las Cumbres Observatory Global Telescope Network, United States

    12 publications · 1.5K citations

    12

    h-index

  4. MM
    M. M. Kasliwal

    California Institute of Technology, United States

    12 publications · 1.8K citations

    12

    h-index

  5. SJ
    S. J. Smartt

    Queen's University Belfast, United Kingdom

    12 publications · 631 citations

    12

    h-index

1–5 of 777

Venues

  1. The Astrophysical Journal

    ApJ · 36 publications · 3.3K citations

    28

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    28 publications · 1.7K citations

    23

    h-index

  3. Astronomy and Astrophysics

    9 publications · 539 citations

    10

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 469 citations

    8

    h-index

  5. Nature

    5 publications · 1.7K citations

    5

    h-index

1–5