A new redback pulsar candidate 4FGL J2054.2+6904
arXiv:2306.17593 · doi:10.1093/mnras/stad1992
Abstract
The Fermi catalogue contains about 2000 unassociated -ray sources. Some of them were recently identified as pulsars, including so called redbacks and black widows, which are millisecond pulsars in tight binary systems with non- and partially-degenerate low-mass stellar companions irradiated by the pulsar wind. We study a likely optical and X-ray counterpart of the Fermi source 4FGL J2054.2+6904 proposed earlier as a pulsar candidate. We use archival optical data as well as Swift/XRT and SRG/eROSITA X-ray data to clarify its nature. Using Zwicky Transient Facility data in and bands spanning over 4.7 years, we find a period of 7.5 h. The folded light curve has a smooth sinusoidal shape with the peak-to-peak amplitude of 0.4 mag. The spectral fit to the optical spectral energy distribution of the counterpart candidate gives the star radius of 0.50.1 and temperature of 5500300 K implying a G2--G9-type star. Its X-ray spectrum is well fitted by an absorbed power law with the photon index of 1.00.3 and unabsorbed flux of erg s cm. All the properties of 4FGL J2054.26904 and its presumed counterpart suggest that it is a member of the redback family.
arXiv commentAccepted for publication in MNRAS, 6 pages, 6 figures
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