PULSE AMPLITUDE DEPENDS ON kHz QPO FREQUENCY IN THE ACCRETING MILLISECOND PULSAR SAX J1808.4-3658
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/2041-8205/798/2/L29/pdf
Reference33 articles.
1. The highest dynamical frequency in the inner region of an accretion disc
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2. The Stochastic X-Ray Variability of the Accreting Millisecond Pulsar IGR J17062–6143;The Astrophysical Journal;2021-11-01
3. Long-term Coherent Timing of the Accreting Millisecond Pulsar IGR J17062–6143;The Astrophysical Journal;2021-05-01
4. Timing the Pulsations of the Accreting Millisecond Pulsar SAX J1808.4–3658 during Its 2019 Outburst;The Astrophysical Journal;2020-07-21
5. On the frequency correlations of low-frequency QPOs with kilohertz QPOs in accreting millisecond X-ray pulsars;Monthly Notices of the Royal Astronomical Society;2019-10-03
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