X-ray Novae

X-Ray Novae is a transient astrophysical phenomenon characterized by a sudden increase in X-ray emission from a compact binary system, distinguished from persistent X-ray sources by its episodic outburst behavior resulting from instabilities in the accretion disk around a stellar-mass black hole or neutron star.

227

Publications

10.4K

Citations

633

Authors

313

Institutions

Publications per year

2017–2026

24

Authors

633

  1. JE
    Jeffrey E. McClintock

    Center for Astrophysics Harvard & Smithsonian, United States

    14 publications · 1.3K citations

    14

    h-index

  2. KM
    K. Mukai

    Goddard Space Flight Center, United States

    10 publications · 390 citations

    10

    h-index

  3. IH
    Izumi Hachisu

    The University of Tokyo, Japan

    10 publications · 266 citations

    10

    h-index

  4. MK
    Mariko Kato

    Keio University, Japan

    11 publications · 264 citations

    10

    h-index

  5. RA
    Ronald A. Remillard

    Massachusetts Institute of Technology, United States

    9 publications · 844 citations

    9

    h-index

1–5 of 633

Venues

  1. The Astrophysical Journal

    ApJ · 80 publications · 4.7K citations

    37

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    47 publications · 2.1K citations

    25

    h-index

  3. Astronomy and Astrophysics

    32 publications · 1.2K citations

    20

    h-index

  4. 10

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 140 citations

    5

    h-index

1–5