Observational Constraints on Superbubble X-ray Energy Budgets

@article{Jaskot2011ObservationalCO,
  title={Observational Constraints on Superbubble X-ray Energy Budgets},
  author={A. Jaskot and D. Strickland and M. Oey and Y. Chu and G. Garc'ia-Segura},
  journal={The Astrophysical Journal},
  year={2011},
  volume={729},
  pages={28}
}
The hot, X-ray-emitting gas in superbubbles imparts energy and enriched material to the interstellar medium (ISM) and generates the hot ionized medium, the ISM's high-temperature component. The evolution of superbubble energy budgets is not well understood, however, and the processes responsible for enhanced X-ray emission in superbubbles remain a matter of debate. We present Chandra ACIS-S observations of two X-ray-bright superbubbles in the Large Magellanic Cloud, DEM L50 (N186), and DEM L152… Expand
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