A NICER discovery of a low-frequency quasi-periodic oscillation in the soft-intermediate state of MAXI J1535–571

Journal article

We present the discovery of a low-frequency ≈5.7 Hz quasi-periodic oscillation (QPO) feature in observations of the black hole X-ray binary MAXI J1535-571 in its soft-intermediate state, obtained in 2017 September-October by the Neutron Star Interior Composition Explorer. The feature is relatively broad (compared to other low-frequency QPOs; quality factor Q ≈ 2) and weak (1.9% rms in 3-10 keV), and is accompanied by a weak harmonic and low-amplitude broadband noise. These characteristics identify it as a weak Type A/B QPO, similar to ones previously identified in the soft-intermediate state of the transient black hole X-ray binary XTE J1550-564. The lag-energy spectrum of the QPO shows increasing soft lags toward lower energies, approaching 50 ms at 1 keV (with respect to a 3-10 keV continuum). This large phase shift has similar amplitude but opposite sign to that seen in Rossi X-Ray Timing Explorer data for a Type B QPO from the transient black hole X-ray binary GX 339-4. Previous phase-resolved spectroscopy analysis of the Type B QPO in GX 339-4 pointed toward a precessing jet-like corona illuminating the accretion disk as the origin of the QPO signal. We suggest that this QPO in MAXI J1535-571 may have the same origin, with the different lag sign depending on the scale height of the emitting region and the observer inclination angle.

Authors: Stevens, AL; Uttley, P; Altamirano, D; Arzoumanian, Z; Bult, P

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: American Astronomical Society
• Journal: Astrophysical Journal Letters
• Volume: 865
• Issue: 2
• Publication date: 2018-09-26
• Acceptance date: 2018-09-14
• DOI: 10.3847/2041-8213/aae1a4
• EISSN: 2041-8213
• ISSN: 2041-8205
• Keywords: X-rays; individual (MAXI J1535); X-rays; binaries; black hole physics; accretion, accretion disks; stars; black holes