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Fig. 8


Simulated transmission for a mixture of gas (10%) plus a dominant dust component: iron gas (black), metallic iron (red), and pyroxene En60Fs40 in both amorphous (green) and crystalline (blue) form. We set a solar abundance and we also simulate the transmission of pure iron gas (black) as a reference. The red shadow represents the noise for the iron metallic model. Top: simulation with Chandra-HETG. Middle: simulation with the XARM-SXS microcalorimeter (see also Paerels et al. 2014). Bottom: simulation with Athena-XIFU (see also Decourchelle et al. 2013).

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