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X-ray spectroscopy (PDF) - SRON

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• UTA = Unresolved<br />

Transition Ar<strong>ray</strong>, blend<br />

of narrow features<br />

• Due to inner-shell<br />

transitions<br />

• Almost no accurate<br />

atomic data available<br />

before Sako et al.<br />

(2001)<br />

The Fe UTA<br />

97<br />

Calculations & Lab measurements<br />

of inner-shell transitions<br />

• Example: oxygen<br />

K-shell transitions (Gu<br />

et al. 2005)<br />

• Lab measurements:<br />

EBIT<br />

• Calculations: FAC<br />

• accurate λ for<br />

O V 1s-2p main line:<br />

uncertainty only 3 mÅ<br />

(50 km/s)<br />

98<br />

Sample spectra<br />

RGS 600 ks, Detmers et al. 2011 (paper III)<br />

Example: AGN outflow Mrk 509<br />

(Detmers et al. 2011)<br />

99<br />

100<br />

More on photoionised plasmas<br />

Photoionised plasmas<br />

• Irradiated plasma<br />

• Two balance equations:<br />

Photons:<br />

Photo-ionisation<br />

Heating by photoelectrons<br />

Electrons:<br />

Radiative<br />

recombination<br />

(electron capture)<br />

Cooling by collisional<br />

excitation (followed<br />

by line radiation)<br />

101<br />

102

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