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X-ray spectroscopy (PDF) - SRON

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Continuum versus line<br />

absorption<br />

Example: O VIII<br />

Continuum absorption<br />

91<br />

92<br />

Line absorption<br />

Sample high-resolution absorption spectra<br />

(Mrk 509, Seyfert galaxy, 600 ks RGS data; Detmers et al. 2011)<br />

93 94<br />

Resonance scattering<br />

Spotlight: Inner-shell transitions<br />

• Alternative to measure<br />

turbulence<br />

• Fe XVII 15.02 to<br />

17.05/17.10 ratio<br />

sensitive to res. scat. (τ<br />

depends on turbulence)<br />

• Currently only RGS can<br />

do it (see also Werner et<br />

al. 2009)<br />

• SXS can map it<br />

Xu et al. 2002, NGC 4636<br />

95<br />

96

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