MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND
We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all contain moderately broad components of FeK-shell emission and are ideal candidates for testing the applicability of a Com...
| المؤلفون الرئيسيون: | , , , , , , |
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| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
Institute of Physics Publishing
2012
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