PoS - Proceedings of Science
Volume 425 - The Multifaceted Universe: Theory and Observations - 2022 (MUTO2022) - Relativistic astrophysics
Long-term X-ray/UV observations of the ultraluminous X-ray source HolmbergII X-1.
K.E. Atapin*, A. Vinokurov, M. Safonova, S. Fabrika and O. Bordoloi
Full text: pdf
Pre-published on: September 16, 2022
Published on: December 14, 2022
Ultraluminous X-ray sources (ULXs) are point-like extra-galactic source with luminosities exceeding the Eddington limit for stellar-mass black holes. The results of our recent observations of one of these sources - Holmberg II X-1 - with the Astrosat observatory prompted us to look at the long-term brightness and spectral variability of this source using the Swift/XRT observations. We found that after being in the state of low variability ($\lesssim2$ times) and hard spectrum ($\Gamma\sim1.8$) for about ten years, the source returned into the state with high variability ($\gtrsim 10$ times ) and a soft spectrum ($\Gamma\sim2.5$). Thus, during the time of the Swift monitoring of more than 15 years, the ULX experienced the state transitions at least 3 times. Also we found that the period of 27 days observed in the variable state and vanished in the steady state appeared again as the source returned to the variable state. Further analysis and modeling are necessary to shed light on the possible mechanisms of the observed state transitions of Holmberg II X-1.
DOI: https://doi.org/10.22323/1.425.0056
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.