A universal average spectral energy distribution for quasars from the optical to the extreme ultravi...
A universal average spectral energy distribution for quasars from the optical to the extreme ultraviolet
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London: Nature Publishing Group UK
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English
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London: Nature Publishing Group UK
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Quasars feature gas swirling towards a supermassive black hole inhabiting a galactic centre. The disk accretion produces enormous amounts of radiation from optical to ultraviolet (UV) wavelengths. Extreme UV (EUV) emission, stemming from the energetic innermost disk regions, has critical implications for the production of broad emission lines in qu...
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A universal average spectral energy distribution for quasars from the optical to the extreme ultraviolet
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TN_cdi_proquest_journals_2901728782
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2901728782
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ISSN
2397-3366
E-ISSN
2397-3366
DOI
10.1038/s41550-023-02088-5