HE0359-3959: An Extremely Radiating Quasar
This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in...
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2017 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/369962 |
| Acceso en línea: | http://hdl.handle.net/10261/369962 |
| Access Level: | acceso abierto |
| Palabra clave: | Quasars: emission lines Quasars: outflows Quasars: individuals HE0359-3959 Quasars: supermassive black holes Galaxy evolution: feedback |
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HE0359-3959: An Extremely Radiating QuasarMartínez-Aldama, Mary LoliOlmo, Ascensión delMarziani, PaolaNegrete, C. AlenkaDultzin, DeborahMartínez Carballo, M. A.Quasars: emission linesQuasars: outflowsQuasars: individuals HE0359-3959Quasars: supermassive black holesGalaxy evolution: feedbackThis is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.We 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 Civ¿1549 emission line. A prominent blueshifted component is also associated with the 1900Å blend, resembling the one observed in Civ¿1549. 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. © 2017 Martínez-Aldama, Del Olmo, Marziani, Negrete, Dultzin and Martínez-CarballoMLM-A acknowledge the postdoctoral grant from the CONACyT. MLM-A, AD, and MAM-C acknowledge financial support from Spanish Ministry for Economy and Competitiveness through grants AYA2013-42227-P and AYA2016-76682-C3-3-1-P.Frontiers MediaConsejo Nacional de Ciencia y Tecnología (México)Ministerio de Economía y Competitividad (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420172024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/369962reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO//AYA2013-42227-Pinfo:eu-repo/grantAgreement/MINECO//AYA2016-76682-C3-3-1-Phttp://dx.doi.org/10.3389/fspas.2017.00029Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3699622026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
HE0359-3959: An Extremely Radiating Quasar |
| title |
HE0359-3959: An Extremely Radiating Quasar |
| spellingShingle |
HE0359-3959: An Extremely Radiating Quasar Martínez-Aldama, Mary Loli Quasars: emission lines Quasars: outflows Quasars: individuals HE0359-3959 Quasars: supermassive black holes Galaxy evolution: feedback |
| title_short |
HE0359-3959: An Extremely Radiating Quasar |
| title_full |
HE0359-3959: An Extremely Radiating Quasar |
| title_fullStr |
HE0359-3959: An Extremely Radiating Quasar |
| title_full_unstemmed |
HE0359-3959: An Extremely Radiating Quasar |
| title_sort |
HE0359-3959: An Extremely Radiating Quasar |
| dc.creator.none.fl_str_mv |
Martínez-Aldama, Mary Loli Olmo, Ascensión del Marziani, Paola Negrete, C. Alenka Dultzin, Deborah Martínez Carballo, M. A. |
| author |
Martínez-Aldama, Mary Loli |
| author_facet |
Martínez-Aldama, Mary Loli Olmo, Ascensión del Marziani, Paola Negrete, C. Alenka Dultzin, Deborah Martínez Carballo, M. A. |
| author_role |
author |
| author2 |
Olmo, Ascensión del Marziani, Paola Negrete, C. Alenka Dultzin, Deborah Martínez Carballo, M. A. |
| author2_role |
author author author author author |
| dc.contributor.none.fl_str_mv |
Consejo Nacional de Ciencia y Tecnología (México) Ministerio de Economía y Competitividad (España) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Quasars: emission lines Quasars: outflows Quasars: individuals HE0359-3959 Quasars: supermassive black holes Galaxy evolution: feedback |
| topic |
Quasars: emission lines Quasars: outflows Quasars: individuals HE0359-3959 Quasars: supermassive black holes Galaxy evolution: feedback |
| description |
This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms. |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017 2024 2024 2024 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/369962 |
| url |
http://hdl.handle.net/10261/369962 |
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Inglés |
| language_invalid_str_mv |
Inglés |
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#PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/MINECO//AYA2013-42227-P info:eu-repo/grantAgreement/MINECO//AYA2016-76682-C3-3-1-P http://dx.doi.org/10.3389/fspas.2017.00029 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Frontiers Media |
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Frontiers Media |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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