Is Superorbital Modulation in SMC X-1 Caused by Absorption in a Warped Precessing Accretion Disk?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab8224/pdf
Reference39 articles.
1. Observations of Accreting Pulsars
2. The super-orbital modulation of supergiant high-mass X-ray binaries
3. Modeling the Precession of the Warped Inner Accretion Disk in the Pulsars LMC X-4 and SMC X-1 with NuSTAR and XMM-Newton
4. Long-term properties of accretion discs in X-ray binaries -- I. The variable third period in SMC X-1
5. SUPERORBITAL PERIODIC MODULATION IN WIND-ACCRETION HIGH-MASS X-RAY BINARIES FROMSWIFTBURST ALERT TELESCOPE OBSERVATIONS
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1. Swift/XRT observations of superorbital modulations in wind-fed supergiant X-ray binaries;Monthly Notices of the Royal Astronomical Society;2023-12-23
2. Spectral Energy Distributions of Southern Binary X-Ray Sources;The Astrophysical Journal Supplement Series;2023-09-01
3. An investigation of the ‘10 keV feature’ in the spectra of accretion powered X-ray pulsars with NuSTAR;Monthly Notices of the Royal Astronomical Society;2023-08-31
4. Clumpy Wind Studies and the Nondetection of a Cyclotron Line in OAO 1657–415;The Astrophysical Journal;2023-03-01
5. Monitoring observations of SMC X-1’s excursions (MOOSE) – II. A new excursion accompanies spin-up acceleration;Monthly Notices of the Royal Astronomical Society;2023-02-06
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