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Haro 5-2: A New Pre-main-sequence Quadruple Stellar System

  • Authors: Bo Reipurth, C. Briceño, T. R. Geballe, C. Baranec, S. Mikkola, A. M. Cody, M. S. Connelley, C. Flores, B. A. Skiff, J. D. Armstrong, N. M. Law, R. Riddle

Bo Reipurth et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 2.

TESS light curves of the combined light from the four components of Haro 5-2 from around 2018 December (Sector 6; top) and around 2020 December (Sector 32; bottom). For Sector 6, the cadence was once every 30 minutes, and for Sector 32, it was once every 10 minutes.

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