File:Müller.camenzind.2004 fe-line-profile.jpg
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Three effects form the line profile. This simulated profile of an iron K line has typical parameters for Seyfert–1 galaxies. The observer is intermediately inclined, the plasma rotates only Keplerian and typical disk sizes r_in = r_ms, r_out = 50 r_g were taken.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 16:03, 27 August 2013 | | 225 × 224 (6 KB) | Odele Straub (Talk | contribs) | Three effects form the line profile. This simulated profile of an iron K line has typical parameters for Seyfert–1 galaxies. The observer is intermediately inclined, the plasma rotates only Keplerian and typical disk sizes r_in = r_ms, r_out = 50 r_g |
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