000095463 001__ 95463 000095463 005__ 20200923100128.0 000095463 0247_ $$2doi$$a10.3389/fspas.2017.00029 000095463 0248_ $$2sideral$$a118463 000095463 037__ $$aART-2017-118463 000095463 041__ $$aeng 000095463 100__ $$0(orcid)0000-0002-7374-3222$$aMartínez-Aldama, M.L.$$uUniversidad de Zaragoza 000095463 245__ $$aHE0359-3959: An extremely radiating quasar 000095463 260__ $$c2017 000095463 5060_ $$aAccess copy available to the general public$$fUnrestricted 000095463 5203_ $$aWe present a multiwavelength spectral study of the quasar HE0359-3959, which has been identified as an extreme radiating source at intermediate redshift (z = 1.5209). Along the spectral range, the different ionic species give information about the substructures in the broad line region. The presence of a powerful outflow with an extreme blueshifted velocity of ~–6,000 ± 500 km s−1 is shown in the Civλ1549 emission line. A prominent blueshifted component is also associated with the 1900Å blend, resembling the one observed in Civλ1549. We detect a strong contribution of very the low–ionization lines, FeII and Near-Infrared Ca II triplet. We find that the physical conditions for the low, intermediate, and high–ionization emission lines are different, which indicate that the emission lines are emitted in different zones of the broad line region. The asymmetries shown by the profiles reveal different forces over emitter zones. The high–ionization region is strongly dominated by radiation forces, which also affect the low and intermediate–ionization emitter region, commonly governed by virial motions. These results support the idea that highly radiating sources host a slim disk. 000095463 536__ $$9info:eu-repo/grantAgreement/ES/MINECO/AYA2013-42227-P$$9info:eu-repo/grantAgreement/ES/MINECO/AYA2016-76682-C3-3-1-P 000095463 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/ 000095463 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion 000095463 700__ $$aOlmo, A. del 000095463 700__ $$aMarziani, P. 000095463 700__ $$aNegrete, C. A. 000095463 700__ $$aDultzin, D. 000095463 700__ $$aMartínez-Carballo, M.A. 000095463 7102_ $$12005$$2595$$aUniversidad de Zaragoza$$bDpto. Matemática Aplicada$$cÁrea Matemática Aplicada 000095463 773__ $$g4 (2017), Art. 29 [5 pp.]$$pFront. astron. space sci.$$tFrontiers in astronomy and space sciences$$x2296-987X 000095463 8564_ $$s768845$$uhttps://zaguan.unizar.es/record/95463/files/texto_completo.pdf$$yVersión publicada 000095463 8564_ $$s34017$$uhttps://zaguan.unizar.es/record/95463/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada 000095463 909CO $$ooai:zaguan.unizar.es:95463$$particulos$$pdriver 000095463 951__ $$a2020-09-23-08:48:36 000095463 980__ $$aARTICLE