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PSR J2032 4127

From Wikipedia, the free encyclopedia

PSR J2032 4127, sometimes abbreviated as J2032, is a pulsar. It is accompanied by a massive Be star named MT91 213 (also 2MASS J20321312 4127243). The system is located in the constellation Cygnus (constellation) at a distance of about 1.4 kpc (~ 4570 al ) from the Sun. The system is part of the Cygnus OB2 association.

It is expected that the coming together of the two stars in early 2018 will generate high-energy phenomena.[1]

The System has an orbital period of around 45-50 yr.[2]

References

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  1. ^ Lyne, A. G; Stappers, B. W; Keith, M. J; Ray, P. S; Kerr, M; Camilo, F; Johnson, T. J (2015). "The binary nature of PSR J2032 4127". Monthly Notices of the Royal Astronomical Society. 451 (1): 581–587. arXiv:1502.01465. Bibcode:2015MNRAS.451..581L. doi:10.1093/mnras/stv236. S2CID 118441808.
  2. ^ Ho (2020). "Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032 4127/MT91 213 on its approach to periastron". Monthly Notices of the Royal Astronomical Society. 464 (1): 1211. arXiv:1609.06328. Bibcode:2017MNRAS.464.1211H. doi:10.1093/mnras/stw2420.
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