Image Details
Caption: Figure 23.
The total spectrum of the [C II]158 μm line (black), presented as in Figure 5, but using the merged PdBI and NOEMA data set. Both the single-Gaussian and double-Gaussian fits are consistent with those performed on the NOEMA data only (see Figure 5). With ΔBIC12 = 4.7 < 10, a broad [C II]158 μm component is only tentatively detected in the merged PdBI and NOEMA data set.
© 2022. The Author(s). Published by the American Astronomical Society.