Compact Stellar Remnants

Compact Stellar Remnants is a type of stellar end-state object characterized by extremely high density and degenerate matter, resulting from the gravitational collapse of a star, and distinguished from other stellar remnants by its small radius and intense gravitational field, such as white dwarfs, neutron stars, and black holes.

287

Publications

24.3K

Citations

859

Authors

480

Institutions

Publications per year

2017–2026

111

Authors

859

  1. GP
    Giuseppe Pagliara

    Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Italy

    7 publications · 381 citations

    7

    h-index

  2. TA
    Tal Alexander

    Weizmann Institute of Science, Israel

    6 publications · 664 citations

    6

    h-index

  3. GA
    G. Abbas

    Islamia University of Bahawalpur, Pakistan

    6 publications · 369 citations

    6

    h-index

  4. MH
    M. Hilker

    European Southern Observatory, Germany

    5 publications · 160 citations

    5

    h-index

  5. AD
    A. Drago

    Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Italy

    5 publications · 195 citations

    5

    h-index

1–5 of 859

Venues

  1. The Astrophysical Journal

    ApJ · 78 publications · 8.3K citations

    48

    h-index

  2. 34

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 16 publications · 887 citations

    13

    h-index

  4. Astronomy and Astrophysics

    11 publications · 590 citations

    10

    h-index

  5. Astrophysics and Space Science

    8 publications · 398 citations

    8

    h-index

1–5