Image Details
Caption: Figure 16.
Demonstration of the XCLASS fits to both the [C II] and [13C II] features toward W3 IRS5. Top: the simultaneous fit in red overlaid on the spectrum in black. Middle: a zoom-in on the spectrum and fits, where the blue shaded curves highlight the XCLASS fit to the [13C II] hyperfine-structure lines. Bottom: individual [C II] foreground absorption components in gray with the self-absorption feature seen near the systemic velocity of the source highlighted in red.
© 2022. The Author(s). Published by the American Astronomical Society.