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Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738

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Abstract

We present the results of our long-term photometric and spectroscopic monitoring with the 1.5-m telescope RTT-150 for the optical counterpart of the high-mass X-ray binary IGR J21343+4738 discovered in 2002 by the INTEGRAL space X-ray observatory. The X-ray source was also repeatedly detected by the telescopes of the SRG observatory during the all-sky surveys in the period 2019–2021. We have investigated the spectroscopic and photometric variabilities of the optical counterpart, a Be star, caused by physical processes in the equatorial disk. The evolution of the equatorial disk parameters over a long time interval of 16 years has been analyzed.

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  1. https://tug.tubitak.gov.tr/tr/icerik/tfosc-tug-faint-object-spectrograph-and-camera

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ACKNOWLEDGMENTS

We are grateful to TÜBİTAK, the Space Research Institute, the Kazan Federal University, and the Academy of Sciences of Tatarstan for their partial support in using RTT-150 (the Russian–Turkish 1.5-m telescope in Antalya). We are grateful to R.Ya. Zhuchkov and S.S. Melnikov for their help in the RTT-150 observations.

Funding

The analysis of the physical parameters of the equatorial disk of the Be star in the system IGR J21343+4738 was supported by RSF grant no. 21-12-00210. The work of E.R. Irtuganov, M.A. Gorbachev, R.I. Gumerov, and N.A. Sakhibullin was supported in part by subsidy no. FZSM-2023-0015 of the Ministry of Education and Science of the Russian Federation allocated to the Kazan Federal University for the State assignment in the sphere of scientific activities.

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Moscow State University, 119234, Moscow, Russia

    E. A. Nikolaeva, I. F. Bikmaev & M. V. Suslikov

  2. Kazan Federal University, 420000, Kazan, Russia

    E. A. Nikolaeva, I. F. Bikmaev, E. N. Irtuganov, M. A. Gorbachev, M. V. Suslikov, R. I. Gumerov & N. A. Sakhibullin

  3. Academy of Sciences of Tatarstan, 420111, Kazan, Russia

    E. N. Irtuganov, M. A. Gorbachev, R. I. Gumerov & N. A. Sakhibullin

Authors
  1. E. A. Nikolaeva
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  2. I. F. Bikmaev
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  3. E. N. Irtuganov
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  4. M. A. Gorbachev
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  6. R. I. Gumerov
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  7. N. A. Sakhibullin
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Correspondence to E. A. Nikolaeva.

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Translated by V. Astakhov

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Nikolaeva, E.A., Bikmaev, I.F., Irtuganov, E.N. et al. Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738. Astron. Lett. 49, 697–705 (2023). https://doi.org/10.1134/S1063773723110075

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  • DOI: https://doi.org/10.1134/S1063773723110075

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