Accretion mode changes in Centaurus X-3
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:200500177/pdf
Reference19 articles.
1. The mass of the neutron star in Centaurus X-3
2. The Long‐Term Light Curves of X‐Ray Binaries Contain Simultaneous Periodic and Random Components
3. Long-term properties of accretion discs in X-ray binaries -- I. The variable third period in SMC X-1
4. Long-term properties of accretion discs in X-ray binaries -- II. Stability of radiation-driven warping
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2. Orbital- and Spin-phase Variability in the X-Ray Emission from the Accreting Pulsar Centaurus X-3;The Astrophysical Journal;2023-02-01
3. Fitting strategies of accretion column models and application to the broadband spectrum of Cen X-3;Astronomy & Astrophysics;2021-12
4. No apparent accretion mode changes detected in Centaurus X-3;Astronomy & Astrophysics;2011-11
5. X-RAY SPECTROSCOPY OF THE HIGH-MASS X-RAY BINARY PULSAR CENTAURUS X-3 OVER ITS BINARY ORBIT;The Astrophysical Journal;2011-08-08
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