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We introduce structure functions, long-standing tools in extra-galactic astronomy, which have been recently applied to studies of young stellar objects. They can characterise the variability in time-series data in a way that doesn’t rely on periodicity. We apply structure functions to analysis of light curves of YSOs in the star forming region NGC 2264.
{"references": ["Sergison, D et al. (2020) Monthly Notices of the Royal Astronomical Society, Volume 491, Issue 4, p.5035-5055", "Venuti, L et al. (2021) The Astronomical Journal, Volume 162, Issue 3, id.101, 27 pp.", "Lakeland, B & Naylor, T (2022) Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 2, pp.2736-2755"]}
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