Optical Observations of the Black Hole Candidate GX 339−4 (V821 Arae)
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference26 articles.
1. The 14.8-h orbital period of GX339-4
2. Optical variability of the black hole candidate GX339-4 (X1659-487, V821 Ara) - limits on periodic modulation
3. GX 339-4 - Black hole or neutron star X-ray binary?
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1. High-resolution X-Ray Spectroscopy of Interstellar Iron toward Cygnus X-1 and GX 339-4;The Astrophysical Journal;2024-04-01
2. Mini‐outburst of black hole X‐ray binary GX 339‐4 in 2004;Astronomische Nachrichten;2024-02
3. Spectral properties of GX 339−4 in the intermediate state using AstroSat observation;Monthly Notices of the Royal Astronomical Society;2023-10-21
4. The prototype X-ray binary GX 339–4: using TeV γ-rays to assess LMXBs as Galactic cosmic ray accelerators;Monthly Notices of the Royal Astronomical Society;2022-01-10
5. State transitions of GX 339-4 during its outburst rising phase;Monthly Notices of the Royal Astronomical Society;2021-09-24
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