File:Müller.camenzind.2004 fe-line-profile.jpg

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Müller.camenzind.2004_fe-line-profile.jpg(225 × 224 pixels, file size: 6 KB, MIME type: image/jpeg)

    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/TimeThumbnailDimensionsUserComment
    current16:03, 27 August 2013Thumbnail for version as of 16:03, 27 August 2013225 × 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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