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

  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},
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… 


Publications of the Astronomical Society of Australia
Robert Innes was one of a select band of amateur astronomers who made the transition to professional ranks towards the end of the nineteenth century. Initially he had a passion for mathematical
The MUSE second-generation VLT instrument
Summary: The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation VLT panoramic integral-field spectrograph currently in manufacturing, assembly and integration phase. MUSE has a field of
Astrophysics of Gaseous Nebulae and Active Galactic Nuclei
Preface Preface to First Edition General Introduction Photoionization Equilibrium Thermal Equilibrium Calculation of Emitted Spectrum Comparison of Theory with Observations Internal Dynamics of
School of Astronomy at the Institute for Research in Fundamental Sciences for its financial support
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