Image Details
Caption: Figure 21.
The total spectrum of the [C II]158 μm line (black), presented as in Figure 5, but using the previous PdBI data, following the methodology used in this paper. Both the single-Gaussian and double-Gaussian fits are consistent with those performed on the NOEMA data only (see Figure 5). With ΔBIC12 = 3.0 < 10, a broad [C II]158 μm component is only tentatively detected.
© 2022. The Author(s). Published by the American Astronomical Society.