The spectral energy distributions of the whole galaxies show the presence of the cold dust component (Tc ~ 20 K) in addition to
the warm dust component (Tw ~ 60 K).
The warmer dust component is spatially correlated well with the [O III] emission and hence likely to be associated with the highly - ionized gas locally heated by intense radiation from the two clusters.
Not exact matches
We deconvolved the cold and
warm dust emission
components spatially by making the best use of the multi-band photometric capability of the FIS.
We propose that the hot
dust is produced by the release of small carbon grains following the disruption of aggregates that originate from the
warm component.