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The Giant Herbig–Haro Flow HH 212 and Associated Star Formation

  • Authors: Bo Reipurth, C. J. Davis, John Bally, A. C. Raga, B. P. Bowler, T. R. Geballe, Colin Aspin, and Hsin-Fang Chiang

2019 The Astronomical Journal 158 107.

  • Provider: AAS Journals

Caption: Figure 8.

GNIRS spectrum of HH 212 IRS-B from Gemini-North. Spectral features are indicated. The spectral region from 1.81 to 1.89 μm (between dotted lines) with strong atmospheric absorption (transmission <20%) has been removed, while the region from 1.89 to 2.05 μm with moderate atmospheric absorption (transmission <80%) is indicated by gray shading.

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