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A Search for Dust in the Outflow of the HH 212 Class 0 Protostellar System

  • Authors: Adele L. Plunkett, Per Bjerkeli, Jon P. Ramsey, Daniel Harsono, Hannah Shoemaker

Adele L. Plunkett et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Histograms of the estimated masses of indicated regions observed with Bands 7 and 9, using Equation (3) and the data in Table 2. Uncertainties in mass are calculated using the rms values (ΔM ∝ rms) and uncertainties in β values, and are shown as black error bars. Left: estimated mass adopting κλ ∝ κλ,0(λ/1 mm)−β, with κλ,0 = 0.078 cm2 g−1 (V. Ossenkopf & T. Henning 1994). Right: estimated mass adopting κλ,0 = 0.35 cm2 g−1 (B. T. Draine 2003a, 2003b). Note the difference in the scaling of the y-axis between panels.

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