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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 9.

H-band spectra of the individual Ba and Bb components resolved with adaptive optics and GNIRS at the Gemini-North 8 m telescope. Wavelength is in microns and flux is in Wm⁻² μm⁻¹.

(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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