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Study of the Be/X-ray binary IGR J21343+4738 physical parameters based on the 15-years monitoring

Published online by Cambridge University Press:  29 August 2024

Evgeniia Nikolaeva Open the ORCID record for Evgeniia Nikolaeva [Opens in a new window]  and
Ilfan Bikmaev
Evgeniia Nikolaeva*
Affiliation:
Kazan (Volga-region) Federal University, Kremlevskaya 18, 420008, Kazan, Russian Federation Academy of Sciences of Tatarstan, Baumana, 20, 420111, Kazan, Russian Federation
Ilfan Bikmaev
Affiliation:
Kazan (Volga-region) Federal University, Kremlevskaya 18, 420008, Kazan, Russian Federation Academy of Sciences of Tatarstan, Baumana, 20, 420111, Kazan, Russian Federation
*
*email: evgeny.nikolaeva@gmail.com
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Abstract

We present the results of our long-term RTT-150 photometric and spectroscopic observations Be optical counterpart of the High-mass X-ray binary IGR J21343+4738.

Keywords

X-rays: binariesstars: emission-lineBestars: individual (IGR J21343+4738)
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 321 - 322
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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References

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