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Extragalactic Astronomy and Cosmology: An Introduction

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5. Active Galactic Nuclei<br />

192<br />

Fig. 5.16. The profile of the broad iron line is caused by<br />

a combination of Doppler shift, relativistic beaming, <strong>and</strong><br />

gravitational redshift. On the left, the observed energy of<br />

the line as a function of position on a rotating disk is indicated<br />

by colors. Here, the energy in the right part of the<br />

disk which is moving towards us is blueshifted, whereas the<br />

left part of the disk emits redshifted radiation. Besides this<br />

Doppler effect, all radiation is redshifted because the photons<br />

must escape from the deep potential well. The smaller<br />

the radius of the emitting region, the larger this gravitational<br />

redshift. The line profile we would obtain from a ring-shaped<br />

section of the disk (dashed ellipses) is plotted in the panels<br />

on the right. The uppermost panel shows the shape of<br />

the line we would obtain if no relativistic effects occurred<br />

besides the non-relativistic Doppler effect. Below, the line<br />

profile is plotted taking the relativistic Doppler effect <strong>and</strong><br />

beaming (see Eq. 5.31) into account. This line profile is<br />

shifted towards smaller energies by gravitational redshift so<br />

that, in combination, the line profile shown at the bottom<br />

results<br />

Fig. 5.17. The ratio of the X-ray spectrum of AGNs <strong>and</strong> a fitted<br />

power law averaged over 53 Type 1 AGNs (left panel) <strong>and</strong> 41<br />

Type 2 AGNs (right panel). The gray <strong>and</strong> black data points<br />

are from two different detectors on-board the XMM-Newton<br />

observatory. In both AGN samples, a broad relativistic iron<br />

line is visible; in the Type 2 AGNs, an additional narrow<br />

line component at 6.4 keV can be identified. The line strength<br />

indicates that the average iron abundance in these sources is<br />

about three times the Solar value

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