Universality in the random walk structure function of luminous quasi-stellar objects

Ji Jia Tang*, Christian Wolf*, John Tonry

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    7 Citations (Scopus)

    Abstract

    Rapidly growing black holes are surrounded by accretion disks that make them the brightest objects in the Universe. Their brightness is known to be variable, but the causes of this are not implied by simple disk models and still debated. Due to the small size of accretion disks and their great distance, there are no resolved images addressing the puzzle. In this work, we study the dependence of their variability on luminosity, wavelength and orbital/thermal timescale. We use over 5,000 of the most luminous such objects with light curves of almost nightly cadence from >5 years of observations by the NASA/ATLAS project, which provides 2 billion magnitude pairs for a structure function analysis. When time is expressed in units of orbital or thermal timescale in thin-disk models, we find a universal structure function, independent of luminosity and wavelength, supporting the model of magneto-rotational instabilities as a main cause. Over a >1 dex range in time, the fractional variability amplitude follows log(A/ A) ≃ 1 / 2 × log(Δ t/ tth). Deviations from the universality may hold clues as to the structure and orientation of disks.

    Original languageEnglish
    Pages (from-to)473-480
    Number of pages8
    JournalNature Astronomy
    Volume7
    Issue number4
    DOIs
    Publication statusPublished - Apr 2023

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