First characterization of a new high-mass X-ray binary in LMC eRASSU J050810.4−660653 with SRG/ART-XC, NuSTAR, and Swift

• Published in: Monthly notices of the Royal Astronomical Society Vol. 514; no. 3; pp. 4018 - 4025
• Main Authors: Salganik, Alexander, Tsygankov, Sergey S, Lutovinov, Alexander A, Mushtukov, Alexander A, Mereminskiy, Ilya A, Molkov, Sergey V, Semena, Andrei N
• Format: Journal Article
• Language: English
• Published: Oxford University Press 28-06-2022
• Subjects: stars: magnetic field; scattering; X-rays: binaries; accretion, accretion discs; pulsars: general; stars: neutron
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stac1608

ABSTRACT
We report results of the first detailed spectral and temporal studies of the recently discovered Be/X-ray binary eRASSU J050810.4−660653 in Large Magellanic Cloud based on the data from the SRG/ART-XC, NuSTAR and Swift/XRT instruments obtained in 2021 December–2022 May in a wide energy range of 0.5–79 keV. Pulsations with the period of 40.5781 ± 0.0004 s were found in the source light curve with the pulsed fraction monotonically increasing with the energy. An estimate of the orbital period of ∼38 d was obtained based on the long-term monitoring of the system. The source spectrum can be well approximated with a power-law model modified by an exponential cutoff at high energies. The pulse phase-resolved spectroscopy shows a strong variation of spectral parameters depending on the phase of a neutron star rotation. We have not found any features connected with the cyclotron absorption line both in the phase-averaged and phase-resolved spectra of eRASSU J050810.4−660653. However, the neutron star magnetic field was estimated around several 1013 G using different indirect methods. Discovered variations of the hardness ratio over the pulse phase is discussed in terms of physical and geometrical properties of the emitting region.