Periodic variability during the X-ray decline of 4U 1636-53
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/361/2/602/18661323/361-2-602.pdf
Reference30 articles.
1. High-energy observations of the state transition of the X-ray nova and black hole candidate XTE J1720-318
2. The Accretion Disk Limit Cycle Model: Toward an Understanding of the Long-Term Behavior of SS Cygni
3. The Properties of X‐Ray and Optical Light Curves of X‐Ray Novae
4. On the correlated spectral and timing properties of 4U 1636–53: An atoll source at high accretion rates
5. X-ray irradiation in low-mass binary systems
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1. Investigation into the reflection properties of the neutron star low-mass X-ray binary 4U 1636–53;Astronomy & Astrophysics;2023-09
2. Long-term Quasiperiodicity in LMXB 4U 1636–536;The Astrophysical Journal;2023-02-01
3. Thermonuclear X-ray bursts from 4U 1636 − 536 observed with AstroSat;Monthly Notices of the Royal Astronomical Society;2021-09-20
4. Evidence of disc reflection in the X-ray spectrum of the neutron star low-mass X-ray binary 4U 1636−536;Monthly Notices of the Royal Astronomical Society;2021-04-09
5. Relation between the properties of the kilohertz quasi-periodic oscillations and spectral parameters in 4U 1636−53;Monthly Notices of the Royal Astronomical Society;2017-07-06
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