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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 ultravi...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2901728782

A universal average spectral energy distribution for quasars from the optical to the extreme ultraviolet

About this item

Full title

A universal average spectral energy distribution for quasars from the optical to the extreme ultraviolet

Author / Creator

Publisher

London: Nature Publishing Group UK

Journal title

Nature astronomy, 2023-12, Vol.7 (12), p.1506-1516

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

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...

Alternative Titles

Full title

A universal average spectral energy distribution for quasars from the optical to the extreme ultraviolet

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2901728782

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2901728782

Other Identifiers

ISSN

2397-3366

E-ISSN

2397-3366

DOI

10.1038/s41550-023-02088-5

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