Probing the Propeller Regime with Symbiotic X-ray Binaries

Fuente: arXiv
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Main Authors: Afonina, M. D., Popov, S. B.
Format: Preprint
Published: 2024
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author Afonina, M. D.
Popov, S. B.
author_facet Afonina, M. D.
Popov, S. B.
contents At the moment, there are two neutron star X-ray binaries with massive red supergiants as donors. De et al. (2023) proposed that the system SWIFT J0850.8-4219 contains a neutron star at the propeller stage. We study this possibility by applying various models of propeller spin-down. We demonstrate that the duration of the propeller stage is very sensitive to the regime of rotational losses. Only in the case of a relatively slow propeller model proposed by Davies and Pringle (1981), the duration of the propeller is long enough to provide a significant probability to observe the system at this stage. Future determination of the system parameters (orbital and spin periods, magnetic field of the compact object, etc.) will allow putting strong constraints on the propeller behavior.
format Preprint
id arxiv_https___arxiv_org_abs_2404_17549
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Probing the Propeller Regime with Symbiotic X-ray Binaries
Afonina, M. D.
Popov, S. B.
High Energy Astrophysical Phenomena
At the moment, there are two neutron star X-ray binaries with massive red supergiants as donors. De et al. (2023) proposed that the system SWIFT J0850.8-4219 contains a neutron star at the propeller stage. We study this possibility by applying various models of propeller spin-down. We demonstrate that the duration of the propeller stage is very sensitive to the regime of rotational losses. Only in the case of a relatively slow propeller model proposed by Davies and Pringle (1981), the duration of the propeller is long enough to provide a significant probability to observe the system at this stage. Future determination of the system parameters (orbital and spin periods, magnetic field of the compact object, etc.) will allow putting strong constraints on the propeller behavior.
title Probing the Propeller Regime with Symbiotic X-ray Binaries
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2404.17549