Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738
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...
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| Published in | Astronomy letters Vol. 49; no. 11; pp. 697 - 705 |
|---|---|
| Main Authors | , , , , , , |
| Format | Journal Article |
| Language | English |
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Moscow
Pleiades Publishing
01.11.2023
Springer Nature B.V |
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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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| AbstractList | 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. |
| Author | Nikolaeva, E. A. Irtuganov, E. N. Gumerov, R. I. Bikmaev, I. F. Suslikov, M. V. Gorbachev, M. A. Sakhibullin, N. A. |
| Author_xml | – sequence: 1 givenname: E. A. surname: Nikolaeva fullname: Nikolaeva, E. A. email: evgeny.nikolaeva@gmail.com organization: Sternberg Astronomical Institute, Moscow State University, Kazan Federal University – sequence: 2 givenname: I. F. surname: Bikmaev fullname: Bikmaev, I. F. organization: Sternberg Astronomical Institute, Moscow State University, Kazan Federal University – sequence: 3 givenname: E. N. surname: Irtuganov fullname: Irtuganov, E. N. organization: Kazan Federal University, Academy of Sciences of Tatarstan – sequence: 4 givenname: M. A. surname: Gorbachev fullname: Gorbachev, M. A. organization: Kazan Federal University, Academy of Sciences of Tatarstan – sequence: 5 givenname: M. V. surname: Suslikov fullname: Suslikov, M. V. organization: Sternberg Astronomical Institute, Moscow State University, Kazan Federal University – sequence: 6 givenname: R. I. surname: Gumerov fullname: Gumerov, R. I. organization: Kazan Federal University, Academy of Sciences of Tatarstan – sequence: 7 givenname: N. A. surname: Sakhibullin fullname: Sakhibullin, N. A. organization: Kazan Federal University, Academy of Sciences of Tatarstan |
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| SubjectTerms | Astronomy Astrophysics and Astroparticles B stars Binary stars Observations and Techniques Optical counterparts (astronomy) Photometry Physics Physics and Astronomy Sky surveys (astronomy) Spectroscopy Telescopes X ray binaries X ray sources X ray stars X-ray astronomy X-rays |
| Title | Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738 |
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