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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 7.

Available photometry of HH 212 IRS-B from 1.6 to 8 μm is plotted as black circles, the surrounding lines indicate the photometric uncertainty. The blue triangles, green squares, and red circles show the same photometry dereddened by AV = 15, 30, and 44 mag. Two blackbody curves for 3916 K (solid curve) and 4570 K (dashed curve) are fitted to the shortest wavelength photometric point for all three dereddened data sets; these temperatures correspond to M0 and K0 giants.

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