Timing Analysis of the 2022 Outburst of SAX J1808.4-3658: Hints of Orbital Decay

Dec 19, 2022
11 pages
Published in:
  • Astrophys.J.Lett. 942 (2023) 2, L40
  • Published: Jan 17, 2023
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Abstract: (IOP)
We present a pulse timing analysis of NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4−3658 during the outburst that started on 2022 August 19. Similar to previous outbursts, after decaying from a peak luminosity of ≃1 × 1036^{36} erg s1^{−1} in about a week, the pulsar entered a ∼1 month long reflaring stage. Comparison of the average pulsar spin frequency during the outburst with those previously measured confirmed the long-term spin derivative of Hz s1^{−1}, compatible with the spin-down torque of a ≈1026^{26} G cm3^{3} rotating magnetic dipole. For the first time in the last twenty years, the orbital phase evolution shows evidence for a decrease of the orbital period. The long-term behavior of the orbit is dominated by an ∼11 s modulation of the orbital phase epoch consistent with a ∼21 yr period. We discuss the observed evolution in terms of a coupling between the orbit and variations in the mass quadrupole of the companion star.
Note:
  • 11 pages, 3 figures, 1 table. Accepted for publication in ApJ Letters