Whether H72.97−69.39’s X-ray spectrum requires both thermal and non-thermal components
Determine whether the X-ray spectrum of H72.97−69.39 necessitates inclusion of both a thermal plasma component and a non-thermal (power-law) component, or whether a single-component model suffices given the current data quality.
References
The diffuse X-ray emission of RCW 38 requires both thermal and non-thermal components to fit the spectra, whereas the weaker signal from H72.97−69.39 does not enable us to distinguish whether both components are necessary to model the data adequately.
— Detection of Diffuse Hot Gas Around the Young, Potential Superstar Cluster H72.97-69.39
(2402.14056 - Webb et al., 21 Feb 2024) in Section 4.2, Comparison to Other Young Star Clusters