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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 9.

(a) An enlargement from the molecular hydrogen image in Figure 3(a) showing a small edge-on disk (encircled). The central star is faintly detected, and here called IRS-C. This new source is not detected by 2MASS or WISE, but is bright in a Herschel 250 μm image. (b) A K-band image of a region ∼38 × 40″ showing the edge-on disk and its illuminating source IRS C. The star 18″ to the NE is nebulous, and so apparently also young. It is here called IRS-D. North is up and east is left.

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