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The Physical Relation between Disc and Coronal Emission in Quasars
We propose a modified version of the observed non-linear relation between the X-ray (2 keV) and the ultraviolet (2,500 Å) emission in quasars (i.e., LX∝LUVγ) which involves the full width at half-maximum, FWHM, of the broad emission line, i.e., LX∝LUVγ^ FWHMβ^. By analyzing a sample of 550 optically...
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| Main Authors: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Frontiers Media S.A.
2018-01-01
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| Colecção: | Frontiers in Astronomy and Space Sciences |
| Assuntos: | |
| Acesso em linha: | http://journal.frontiersin.org/article/10.3389/fspas.2017.00066/full |
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