Role of Thermal and Non-thermal Processes in the ISM of Magellanic Clouds

@inproceedings{Hassani2021RoleOT,
  title={Role of Thermal and Non-thermal Processes in the ISM of Magellanic Clouds},
  author={Hossain Hassani and Fatemeh S Tabatabaei and Annie Hughes and J{\'e}r{\'e}my Chastenet and Anna F. McLeod and Eva Schinnerer and Sorbonne University and Institute for Research in Fundamental Sciences and Cnrs and Universit'e de Toulouse and University of Southern California and G. Wegner Cornell University and University of California Berkeley and Durham University and Max-Planck-Institut fur Astronomie},
  year={2021}
}
The radio continuum emission is a dust-unbiased tracer of both the thermal and non-thermal processes in the interstellar medium. We present new maps of the free-free and synchrotron emission in the Magellanic Clouds (MCs) at 0.166, 1.4, and 4.8 GHz with no prior assumption about the radio non-thermal spectrum. The maps were constructed using a de-reddened Hα map as a template for the thermal radio emission, which we subtract from maps of the total radio continuum emission. To de-redden the H… 

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