A two-sided but significantly beamed jet in the supercritical accretion quasar IRAS F11119+3257
A two-sided but significantly beamed jet in the supercritical accretion quasar IRAS F11119+3257
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Highly accreting quasars are quite luminous in the X-ray and optical regimes. While, they tend to become radio quiet and have optically thin radio spectra. Among the known quasars, IRAS F11119+3257 is a supercritical accretion source because it has a bolometric luminosity above the Eddington limit and extremely powerful X-ray outflows. To probe its...
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A two-sided but significantly beamed jet in the supercritical accretion quasar IRAS F11119+3257
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TN_cdi_proquest_journals_2383283550
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2383283550
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2003.11427