Image Details
Caption: Figure 7.
Zoomed-in view of Source 2 in the LMC. Source 2 is marked as star in these plots. The top panel shows the maximum brightness temperature (TB,max) after we smooth each emission spectrum in the data cube by a Gaussian kernel of standard deviation of three channels. The bottom-left panel provides a further zoomed-in view of the square region marked in the top panel. The bottom-right panel presents the velocity corresponding to the TB,max, showing only regions where TB,max > 6 K.
© 2025. The Author(s). Published by the American Astronomical Society.