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dc.rights.licenseAtribución-CompartirIgual 4.0 Internacional
dc.contributor.advisorHiguera Garzón, Mario Armando
dc.contributor.authorPerdomo Rodríguez, Martha Morelia
dc.date.accessioned2022-08-12T13:34:55Z
dc.date.available2022-08-12T13:34:55Z
dc.date.issued2022-06-24
dc.identifier.urihttps://repositorio.unal.edu.co/handle/unal/81862
dc.descriptionilustraciones, gráficas, tablas
dc.description.abstractLos mapeos de reverberación han sido la base para encontrar relaciones entre el tamaño de la región de líneas anchas (BLR Broad Line Region por sus siglas en Inglés) y sus luminosidades en las bandas del continuo óptico, ultravioleta, rayos X y líneas de emisión de Balmer. Esta tesis describe y aplicó la técnica del mapeo de reverberación con el fin de conocer la metodología para encontrar el tamaño de la región de líneas anchas, metodología que hace uso de las variaciones correlacionadas entre el continuo y las líneas de emisión [Kaspi, 2000]. Esta tesis partió de la información del tamaño de la región de líneas anchas del grupo de galaxias del trabajo de [Kaspi, 2005] e hizo uso de la base de datos del NED para encontrar datos de luminosidades de estas galaxias en la banda de rayos X duros, con el objetivo de estimar una relación entre el tamaño de la región de líneas anchas y las luminosidades en la banda de rayos X en el rango de 10 keV - 195 KeV, aplicando uno de los métodos de regresión lineal informado en [Kaspi, 2005]. (Texto tomado de la fuente)
dc.description.abstractReverberation mappings have been the basis for fnding relationships between the size of the broad line region (BLR) and its luminosities in the bands of the optical continuum, ultraviolet, X-rays and Balmer emission lines. This thesis describes and applied the reverberation mapping technique in order to know the methodology to fnd the size of the broad line region, methodology that does use of the correlated variations between the continuum and the emission lines [Kaspi, 2000]. This thesis started from the information on the size of the broad line region of the group of galaxies from the work of [Kaspi, 2005] and made use of the NED database to fnd luminosity data of these galaxies in the hard X-ray band, in order to estimate a relationship between the size of the broad line region and the luminosities in the band of X-rays in the range of 10 keV - 195 KeV, applying one of the regression methods linear reported in [Kaspi, 2005] (Text taken fron the source)
dc.format.extentxiv, 73 páginas
dc.format.mimetypeapplication/pdf
dc.language.isospa
dc.publisherUniversidad Nacional de Colombia
dc.rights.urihttp://creativecommons.org/licenses/by-sa/4.0/
dc.subject.ddc520 - Astronomía y ciencias afines
dc.titleEstimación del tamaño de la BLR usando la emisión de rayos X de alta energía
dc.typeTrabajo de grado - Maestría
dc.type.driverinfo:eu-repo/semantics/masterThesis
dc.type.versioninfo:eu-repo/semantics/acceptedVersion
dc.publisher.programBogotá - Ciencias - Maestría en Ciencias - Astronomía
dc.description.degreelevelMaestría
dc.description.degreenameMagíster en Ciencias - Astronomía
dc.description.researchareaNúcleos Activos de Galaxias
dc.identifier.instnameUniversidad Nacional de Colombia
dc.identifier.reponameRepositorio Institucional Universidad Nacional de Colombia
dc.identifier.repourlhttps://repositorio.unal.edu.co/
dc.publisher.departmentObservatorio Astronómico Nacional
dc.publisher.facultyFacultad de Ciencias
dc.publisher.placeBogotá, Colombia
dc.publisher.placeBogotá, Colombia
dc.publisher.branchUniversidad Nacional de Colombia - Sede Bogotá
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dc.rights.accessrightsinfo:eu-repo/semantics/openAccess
dc.subject.proposalGalaxias
dc.subject.proposalGalaxias:activas
dc.subject.proposalGalaxias: nucleo
dc.subject.proposalCuasares:líneas de emisión
dc.subject.proposalGalaxias:Seyfert
dc.subject.proposalGalaxias: rayos X
dc.subject.proposalGalaxies:active
dc.subject.proposalGalaxies: nuclei
dc.subject.proposalQuasars:emission lines
dc.subject.proposalGalaxies:Seyfert
dc.subject.proposalGalaxies: X rays
dc.title.translatedBLR size estimation using high-energy X-ray emission
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dcterms.audience.professionaldevelopmentEstudiantes
dcterms.audience.professionaldevelopmentGrupos comunitarios
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Atribución-CompartirIgual 4.0 InternacionalEsta obra está bajo licencia internacional Creative Commons Reconocimiento-NoComercial 4.0.Este documento ha sido depositado por parte de el(los) autor(es) bajo la siguiente constancia de depósito