A rare outburst from the stealthy BeXRB system Swift J0549.7-6812

التفاصيل البيبلوغرافية
العنوان: A rare outburst from the stealthy BeXRB system Swift J0549.7-6812
المؤلفون: Coe, M. J., Kennea, J. A., Monageng, I. M., Buckley, D. A. H., Udalski, A., Evans, P. A.
سنة النشر: 2023
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - High Energy Astrophysical Phenomena
الوصف: Swift J0549.7-6812 is an Be/X-ray binary system (BeXRB) in the Large Magellanic Cloud (LMC) exhibiting a 6s pulse period. Like many such systems the variable X-ray emission is believed to be driven by the underlying behaviour of the mass donor Be star. In this paper we report on X-ray observations of the brightest known outburst from this system which reached a luminosity of 8 x 10^37 erg/s. These observations are supported by contemporaneous optical photometric observations, the first reported optical spectrum, as well as several years of historical data from OGLE and GAIA. The latter strongly suggest a binary period of 46.1d. All the observational data indicate that Swift J0549.7-6812 is a system that spends the vast majority of its time in X-ray quiescence, or even switched off completely. This suggests that occasional observations may easily miss it, and many similar systems, and thereby underestimate the massive star evolution numbers for the LMC.
Comment: 7 pages, 11 figures
نوع الوثيقة: Working Paper
DOI: 10.1093/mnras/stad1987
URL الوصول: http://arxiv.org/abs/2306.17098
رقم الأكسشن: edsarx.2306.17098
قاعدة البيانات: arXiv