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VELOCITY-RESOLVED HOT WATER EMISSION DETECTED TOWARD HL TAU WITH THE SUBMILLIMETER ARRAY

  • Authors: Lars E. Kristensen, Joanna M. Brown, David Wilner, and Colette Salyk

2016 The Astrophysical Journal Letters 822 L20.

  • Provider: AAS Journals

Caption: Figure 2.

H2O ﹩{10}_{\mathrm{2,9}}﹩–9﹩{}_{\mathrm{3,6}}﹩ spectrum toward HL Tau (red) and co-added 13CO v = 1–0 (4.7 μm) line emission (blue) toward the same source (Herczeg et al. 2011). The calibrator spectrum of 3c120 is shown for comparison (cyan). Gaussians are fitted to the HL Tau line profiles (cyan), and the baselines are shown (green); the source velocity is marked in magenta. The 13CO spectrum has been offset for clarity, the units are arbitrary for this spectrum, and the deep envelope self-absorption is masked out. The H2O spectra for both HL Tau and 3c120 are obtained over the same region where emission >3σ and r < 5″ (Figure 1).The data used to create this figure are available.

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