Near-periodical spin period evolution in the binary system LMC X-4
Abstract
In this paper, we investigated the long-term evolution of the pulse period in the high-mass X-ray binary LMC X-4 by taking advantage of more than 43 yr of measurements in the X-ray domain. Our analysis revealed for the first time that the source is displaying near-periodical variations of its spin period on a time-scale of roughly 6.8 yr, making LMC X-4 one of the known binary systems showing remarkable long-term spin torque reversals. We discuss different scenarios to interpret the origin of these torque reversals.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- January 2017
- DOI:
- arXiv:
- arXiv:1610.09561
- Bibcode:
- 2017MNRAS.464.2039M
- Keywords:
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- accretion;
- accretion discs;
- stars: individual: LMC X-4;
- X-rays: binaries;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- doi:10.1093/mnras/stw2429