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A NICER look at the state transitions of the black hole candidate MAXI J1535-571 during its reflares

Cúneo, V. A., Alabarta, K., Zhang, L., Altamirano, D., Méndez, M., Padilla, M. A., Remillard, R., Homan, J., Steiner, J. F., Combi, J. A., Muñoz-Darias, T., Gendreau, K. C., Arzoumanian, Z., Stevens, A. L., Loewenstein, M., Tombesi, F., Bult, P., Fabian, A. C., Buisson, D. J. K., Neilsen, J. & Basak, A., Aug-2020, In : Monthly Notices of the Royal Astronomical Society. 496, 2, p. 1001-1012 12 p.

Research output: Contribution to journalArticleAcademicpeer-review

  • V. A. Cúneo
  • K. Alabarta
  • L. Zhang
  • D. Altamirano
  • M. Méndez
  • M. Armas Padilla
  • R. Remillard
  • J. Homan
  • J. F. Steiner
  • J. A. Combi
  • T. Muñoz-Darias
  • K. C. Gendreau
  • Z. Arzoumanian
  • A. L. Stevens
  • M. Loewenstein
  • F. Tombesi
  • P. Bult
  • A. C. Fabian
  • D. J. K. Buisson
  • J. Neilsen
  • A. Basak

The black hole candidate and X-ray binary MAXI J1535-571 was discovered in 2017 September. During the decay of its discovery outburst, and before returning to quiescence, the source underwent at least four reflaring events, with peak luminosities of similar to 10(35-36) erg s(-1) (d/4.1 kpc)(2). To investigate the nature of these flares, we analysed a sample of NICER (Neutron star Interior Composition Explorer) observations taken with almost daily cadence. In this work, we present the detailed spectral and timing analysis of the evolution of the four reflares. The higher sensitivity of NICER at lower energies, in comparison with other X-ray detectors, allowed us to constrain the disc component of the spectrum at similar to 0.5 keV. We found that during each reflare the source appears to trace out a q-shaped track in the hardness-intensity diagram similar to those observed in black hole binaries during full outbursts. MAXI J1535 -571 transits between the hard state (valleys) and softer states (peaks) during these flares. Moreover, the Comptonized component is undetected at the peak of the first reflare, while the disc component is undetected during the valleys. Assuming the most likely distance of 4.1 kpc, we find that the hard-to-soft transitions take place at the lowest luminosities ever observed in a black hole transient, while the soft-to-hard transitions occur at some of the lowest luminosities ever reported for such systems.

Original languageEnglish
Pages (from-to)1001-1012
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume496
Issue number2
Publication statusPublished - Aug-2020

    Keywords

  • accretion, accretion discs, black hole physics, stars: individual: MAXI J1535-571, X-rays: binaries, X-RAY BINARY, QUASI-PERIODIC OSCILLATIONS, ENHANCED MASS-TRANSFER, DWARF-NOVA OUTBURSTS, LIGHT CURVES, NEUTRON-STAR, GAMMA-RAY, TRANSIENT XTE-J1650-500, SAX J1808.4-3658, GX 339-4

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