paper

Nature of 4FGL J2249.4+6229: Evidence for a redback system with a cool companion and low X-ray and -ray luminosities

arXiv:2605.22271 · doi:10.1093/mnras/stag971

Abstract

We report the identification of the likely X-ray and optical counterpart to the unassociated Fermi source 4FGL J2249.4+6229. To clarify its nature, we investigate the X-ray data from Swift/XRT and SRG/eROSITA as well as photometric data from optical catalogues and archival spectroscopic data from the Gemini-North telescope. Using Zwicky Transient Facility data spanning over 6.6 yr, we confirmed a period of 5.6 h likely associated with the orbital motion in a binary system. The folded light curves have a smooth sinusoidal shape with two peaks per period and the amplitude of 0.2 mag. The X-ray spectra of the source are well fitted by an absorbed power law with the photon index of 2.0 and unabsorbed flux of 1.4 erg s cm. All these together with the X-ray to optical flux ratio of 0.2 implies that 4FGL J2249.4+6229 is a promising redback candidate. Fitting the optical light curves with the direct heating model, we obtained the companion mass of 0.5 M and temperature of 3600 K implying an M-type star. This places it among the coldest and most massive companions known in redback systems.Optical spectra confirms the M-type star and shows the broad asymmetric H emission line. For the distance of 500--550 pc derived from the optical data, the source can be the redback with the lowest X-ray and -ray luminosities.

8 pages, 5 figures, accepted for publication in MNRAS

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