2022
DOI: 10.1093/mnras/stac1608
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First characterization of a new high-mass X-ray binary in LMC eRASSU J050810.4−660653 with SRG/ART-XC, NuSTAR, and Swift

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 LMC based on the data from the SRG/ART-XC, NuSTAR and Swift/XRT instruments obtained in December 2021 - May 2022 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 days was obtained based on the… Show more

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Cited by 4 publications
(4 citation statements)
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“…The source became brightest at the end of eRASS4/beginning of eRASS5 when it was detected by Mikhail Pavlinsky ART-XC (Pavlinsky et al 2021), the hard X-ray instrument on board SRG. A NuS-TAR observation independently revealed the pulsations of eRASSU J050810.4-660653 (Salganik et al 2022).…”
Section: Introductionmentioning
confidence: 98%
See 1 more Smart Citation
“…The source became brightest at the end of eRASS4/beginning of eRASS5 when it was detected by Mikhail Pavlinsky ART-XC (Pavlinsky et al 2021), the hard X-ray instrument on board SRG. A NuS-TAR observation independently revealed the pulsations of eRASSU J050810.4-660653 (Salganik et al 2022).…”
Section: Introductionmentioning
confidence: 98%
“…The first scans were performed during a test phase (named eRASS0) before the official start of the all-sky survey (MJD 58828) with eRASS1 and then around the formal transitions of eRASS1-eRASS2, eRASS2-eRASS3, eRASS3-eRASS4, and eRASS4-eRASS5. The red and green dashed lines mark the beginning of the XMM-Newton and NuSTAR observations(Salganik et al 2022;Haberl et al 2021), respectively.…”
mentioning
confidence: 99%
“…The source became brightest at the end of eRASS4/beginning of eRASS5 when it was detected by Mikhail Pavlinsky ART-XC (Pavlinsky et al 2021), the hard X-ray instrument on board SRG. A NuSTAR observation independently revealed the pulsations of eRASSU J050810.4−660653 (Salganik et al 2022).…”
Section: Introductionmentioning
confidence: 99%
“…The first scans were performed during a test phase (named eRASS0) before the official start of the all-sky survey (MJD 58828) with eRASS1 and then around the formal transitions of eRASS1-eRASS2, eRASS2-eRASS3, eRASS3-eRASS4, and eRASS4-eRASS5. The red and green dashed lines mark the beginning of the XMM-Newton and NuSTAR observations(Salganik et al 2022;Haberl et al 2021), respectively.…”
mentioning
confidence: 99%