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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 3.

Left: spectral energy distribution from SIMBAD of the integrated light from the Haro 5-2 quadruple with data from SkyMapper, the Sloan Digital Sky Survey, PanSTARRS, Johnson, the Two Micron All Sky Survey, AKARI, and WISE. Right: WISE images with Haro 5-2, 5-3, and 5-4 marked. The field is about 0.84 pc wide at the distance of Haro 5-2.

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