Image Details
Caption: Figure 6.
Fitting results of H2 rotational emission lines assuming a continuous power-law distribution of temperature T for apertures in the three targets with markers the same as in Figure 3. The ranges of the best-fit temperature distribution index n and low-end temperature T l for ESO137-G034 and the other two targets are indicated above and below the fitting curves, respectively.
© 2024. The Author(s). Published by the American Astronomical Society.