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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 5.

High-resolution spectra of the Hα line of the Haro 5-2A and B components, obtained with the SOAR GHTS on UT 2021-11-19. Upper panel: spectrum of the M2.5 WTTS Haro 5-2A. Lower panel: spectrum of the accreting M3-type CTTS Haro 5-2B. The vertical dashed line is set at the rest wavelength for Hα (6562.8 Å). The blue horizontal dashed line indicates the full width of the Hα profile at 10% of its full height (White & Basri 2003).

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)

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