Identification and characterization of optical and X-ray Supernova Remnants

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dc.contributor.advisorKopsacheili, Maria
dc.contributor.advisorAnastasopoulou, Konstantina
dc.contributor.authorMusté Ferré, Pol
dc.date.accessioned2025-09-12T14:38:53Z
dc.date.available2025-09-12T14:38:53Z
dc.date.issued2025-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2025, Tutores: Maria Kopsacheili, Konstantina Anastasopoulouca
dc.description.abstractThis paper presents a multi-wavelength analysis of supernova remnants (SNRs) in the galaxies NGC 5068 and NGC 628, based on archival optical data from MUSE and X-ray observations from Chandra. SNR candidates are identified through emission-line diagnostics and the selection is performed by established criteria. Extinction-corrected fluxes allow the derivation of luminosities, densities, and shock velocities. Using the optical data, a comparison between the two galaxies is carried out to identify any trends. Additionally, the X-ray counterparts of the optical candidate SNRs are identified and their properties are presentedca
dc.format.extent10 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/223136
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Musté, 2025
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física
dc.subject.classificationSupernovescat
dc.subject.classificationRaigs Xcat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherSupernovaeeng
dc.subject.otherX-rayseng
dc.subject.otherBachelor's theseseng
dc.titleIdentification and characterization of optical and X-ray Supernova Remnantseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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