Precessing And Wobbling Accretion Disk in X-Ray Pulsar Her X-1 In M. N. Pavlinsky ART-XC Telescope Observations
We present the results of observation of LMXBs Her X-1 by the Pavlinsky ART-XC telescope onboard the Spectrum-Roentgen-Gamma(SRG) observatory in the 4-25 keV energy band near the moment of the main turn-on. The orbital phase of opening the X-ray source by accretion disk was determined φb ≈ 0.25. The direct observational evidence of the nutation of the bend incline precessing accretion disk in the Her X-1 system with the period of 0.87 days was retrieved from the analysis of the X-ray flux variability. The pulsations in the X-ray emission was detected at orbital phase φb ≈ 0.77 in the nutational variations of the flux before the main turn-on.
Authors
- N. I. Shakura (ORCID: https://orcid.org/0000-0002-5672-9517)
- V. M. Revnivtsev
Institutions
- Space Research Institute (RU)
- Astronomical Institute of the Slovak Academy of Sciences (SK)
Publication Details
- Published
- 2025-01-01
- DOI
- https://doi.org/10.15826/b978-5-7996-3986-0.31
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00