Consistency between X-ray and UV–optical reverberation measurements in NGC 5548
Context. The hard X-ray-emitting hot corona is a key component of active galaxies. Constraints on the hot corona height can be derived from reverberation studies in both the X-ray and optical bands. Aims. X-ray reverberation mapping (X-ray RM) studies often suggest a very low corona height, whereas...
Furkejuvvon:
| Váldodahkkit: | , , , , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
EDP Sciences
2026-07-01
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| Ráidu: | Astronomy & Astrophysics |
| Fáttát: | |
| Liŋkkat: | https://www.aanda.org/articles/aa/full_html/2026/07/aa58775-25/aa58775-25.html |
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