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Panchromatic modeli...
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Fan, Lulu,1982Shandong University
(författare)
Panchromatic modeling of the extremely luminous dust-obscured quasars at the cosmic noon
- Artikel/kapitelEngelska2019
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Nummerbeteckningar
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LIBRIS-ID:oai:research.chalmers.se:2cc3116e-3a79-43ce-92d0-54c69d665363
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https://doi.org/10.1017/S1743921319001352DOI
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https://research.chalmers.se/publication/530596URI
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Språk:engelska
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Sammanfattning på:engelska
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Ämneskategori:kon swepub-publicationtype
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Ämneskategori:ref swepub-contenttype
Anmärkningar
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The massive galaxies and their central supermassive black holes (SMBHs) co-evolution scenario proposes that a gas-rich major merger can trigger the central starburst and feeding the SMBH accretion, and then star formation is eventually quenched by quasar feedback. In this evolutionary sequence, dust-obscured quasars may represent the critical transition phase between starburst and unobscured quasars. Modeling the panchromatic emission of these hidden monsters provides a unique way to explore their physical properties and therefore the co-evolution between SMBHs and their hosts. However, most of modelling methods are not suitable for the extremely luminous systems with obscured Active Galactic Nucleus (AGN) emission. Here we present two case studies of panchromatic modeling of the extremely luminous dust-obscured quasars at the cosmic noon.
Ämnesord och genrebeteckningar
Biuppslag (personer, institutioner, konferenser, titlar ...)
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Han, YunkunChinese Academy of Sciences
(författare)
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Knudsen, Kirsten Kraiberg,1976Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)kraiberg
(författare)
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Shandong UniversityChinese Academy of Sciences
(creator_code:org_t)
Sammanhörande titlar
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Ingår i:Proceedings of the International Astronomical Union15:S341, s. 268-2701743-92131743-9221
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