A UV to X-Ray View of Soft Excess in Type 1 Active Galactic Nuclei. II. Broadband Correlations
The physical origin of soft X-ray excess (SE) is a long-lasting question, with two prevailing theories—“warm corona” and “ionized reflection”—dominating the discussion. In the warm corona scenario, SE originates from upscattered disk photons and should therefore correlate strongly with UV emission....
में बचाया:
| मुख्य लेखकों: | , , , , , , , |
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| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
IOP Publishing
2025-01-01
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| श्रृंखला: | The Astrophysical Journal |
| विषय: | |
| ऑनलाइन पहुंच: | https://doi.org/10.3847/1538-4357/ae1734 |
| टैग: |
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