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7DT Insight: Variability in Young Stellar Objects

  • Authors: Mi-Ryang Kim, Jeong-Eun Lee, Myungshin Im, Jinho Lee, Ji Hoon Kim, Seo-Won Chang, Gregory S. H. Paek, Hyeonho Choi, Donggeun Tak, Donghwan Hyun, Won-Hyeong Lee, Hyeyoon Lee, ShinGeon Kim, S. Thomas Megeath

Mi-Ryang Kim et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Comparison of a representative source classified as nonvariable in our two-night 7DT analysis and a representative variable source. Panel (a) shows ID 708 (2MASS J05365602-0503066), which we classify as nonvariable based on the present two-night 7DT data. Panel (b) shows ID 421 (MY Ori), which we classify as variable in our 7DT data and which is also known in the literature as an Orion variable. In both panels, observations from 2024 March 23 and March 24, are denoted by gray and red circles, respectively, and error bars represent 1σ photometric uncertainties.

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