Image Details
Caption: Figure 9.
Example of the spectral line fitting for G286c5. Here we use one Gaussian component to fit the spectra of ﹩{{\rm{N}}}_{2}{{\rm{D}}}^{+}﹩(3–2), ﹩{\mathrm{DCO}}^{+}﹩(3–2), and ﹩\mathrm{DCN}﹩(3–2) and two components for C18O(2–1).
© 2020. The American Astronomical Society. All rights reserved.