PI: Thomas Reiprich and Marcus Brueggen

​We propose to study the radio properties of X-ray selected galaxy clusters. This includes studies
of radio haloes, radio relics, tailed radio galaxies, as well as cluster central radio AGN and their
correlation with morphological X-ray parameters. The X-ray and radio views of galaxy clusters
are highly complementary, tracing the hot thermal and relativistic particle populations,
respectively.

PI: Manami Sasaki (ECAP) 

​Stellar winds of massive stars and supernova explosions cause interstellar strong shock waves that expands into the ambient interstellar medium (ISM). A combination of the effect of stellar winds of many stars and supernova remnants (SNRs) forms large structures in the ISM called superbubbles. In the shock waves, interstellar gas is ionised and heated to very high temperatures and particles are accelerated to relativistic energies. In SNRs, heavier elements produced in the progenitor star are expelled into the ISM. We will combine multi-wavelength data of SNRs and superbubbles in the Magellanic Clouds from radio to X-rays to study the interaction between the interstellar shock waves and the ISM and the chemical enrichment of these satellite galaxies of the Milky Way.
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PI:  Vanessa Moss (CASS/CSIRO)

PI:  Gemma Anderson (Curtin)