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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.

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Background

The paper fits H72.97−69.39’s X-ray spectrum with either a single thermal plasma or a single power-law model, both yielding statistically acceptable fits, but the limited net counts preclude robust multi-component modeling.

In comparing to RCW 38, where both thermal and non-thermal components are required, the authors explicitly state they cannot determine whether both components are needed for H72.97−69.39, leaving the spectral composition unresolved.

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