PKS 1622-253: A weakly accreting, powerful gamma-ray source
- Autores
- Punsly, Brian; Rodríguez, Luis F.; Tingay, Steven J.; Cellone, Sergio Aldo
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We discuss new deep radio observations of PKS 1622-253 and their implications for the energetics of the central engine that powers this strong high-energy gamma-ray source. Combining archival infrared and optical measurements with new millimeter observations, we show that even though the accretion flow in PKS 1622-253 is underluminous by quasar standards, a powerful superluminal jet is launched with a higher kinetic luminosity than most EGRET blazars. Only a few percent of the total jet kinetic luminosity is required to power even the most powerful gamma-ray flares that are observed. The implication is that a high-accretion system is not required in order to power the strongest high-energy gamma-ray sources.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Accretion, accretion disks
Black hole physics
Galaxies: active
Galaxies: jets
Quasars: general
Quasars: individual (PKS 1622-253) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84362
Ver los metadatos del registro completo
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PKS 1622-253: A weakly accreting, powerful gamma-ray sourcePunsly, BrianRodríguez, Luis F.Tingay, Steven J.Cellone, Sergio AldoCiencias AstronómicasAccretion, accretion disksBlack hole physicsGalaxies: activeGalaxies: jetsQuasars: generalQuasars: individual (PKS 1622-253)We discuss new deep radio observations of PKS 1622-253 and their implications for the energetics of the central engine that powers this strong high-energy gamma-ray source. Combining archival infrared and optical measurements with new millimeter observations, we show that even though the accretion flow in PKS 1622-253 is underluminous by quasar standards, a powerful superluminal jet is launched with a higher kinetic luminosity than most EGRET blazars. Only a few percent of the total jet kinetic luminosity is required to power even the most powerful gamma-ray flares that are observed. The implication is that a high-accretion system is not required in order to power the strongest high-energy gamma-ray sources.Facultad de Ciencias Astronómicas y Geofísicas2005info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfL93-L96http://sedici.unlp.edu.ar/handle/10915/84362enginfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/498307info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:14Zoai:sedici.unlp.edu.ar:10915/84362Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:15.25SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
title |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
spellingShingle |
PKS 1622-253: A weakly accreting, powerful gamma-ray source Punsly, Brian Ciencias Astronómicas Accretion, accretion disks Black hole physics Galaxies: active Galaxies: jets Quasars: general Quasars: individual (PKS 1622-253) |
title_short |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
title_full |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
title_fullStr |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
title_full_unstemmed |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
title_sort |
PKS 1622-253: A weakly accreting, powerful gamma-ray source |
dc.creator.none.fl_str_mv |
Punsly, Brian Rodríguez, Luis F. Tingay, Steven J. Cellone, Sergio Aldo |
author |
Punsly, Brian |
author_facet |
Punsly, Brian Rodríguez, Luis F. Tingay, Steven J. Cellone, Sergio Aldo |
author_role |
author |
author2 |
Rodríguez, Luis F. Tingay, Steven J. Cellone, Sergio Aldo |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Accretion, accretion disks Black hole physics Galaxies: active Galaxies: jets Quasars: general Quasars: individual (PKS 1622-253) |
topic |
Ciencias Astronómicas Accretion, accretion disks Black hole physics Galaxies: active Galaxies: jets Quasars: general Quasars: individual (PKS 1622-253) |
dc.description.none.fl_txt_mv |
We discuss new deep radio observations of PKS 1622-253 and their implications for the energetics of the central engine that powers this strong high-energy gamma-ray source. Combining archival infrared and optical measurements with new millimeter observations, we show that even though the accretion flow in PKS 1622-253 is underluminous by quasar standards, a powerful superluminal jet is launched with a higher kinetic luminosity than most EGRET blazars. Only a few percent of the total jet kinetic luminosity is required to power even the most powerful gamma-ray flares that are observed. The implication is that a high-accretion system is not required in order to power the strongest high-energy gamma-ray sources. Facultad de Ciencias Astronómicas y Geofísicas |
description |
We discuss new deep radio observations of PKS 1622-253 and their implications for the energetics of the central engine that powers this strong high-energy gamma-ray source. Combining archival infrared and optical measurements with new millimeter observations, we show that even though the accretion flow in PKS 1622-253 is underluminous by quasar standards, a powerful superluminal jet is launched with a higher kinetic luminosity than most EGRET blazars. Only a few percent of the total jet kinetic luminosity is required to power even the most powerful gamma-ray flares that are observed. The implication is that a high-accretion system is not required in order to power the strongest high-energy gamma-ray sources. |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/84362 |
url |
http://sedici.unlp.edu.ar/handle/10915/84362 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-637X info:eu-repo/semantics/altIdentifier/doi/10.1086/498307 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf L93-L96 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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