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The Van der Laan extragalactic emission model applied to GRS 1915+105

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dc.contributor Paredes i Poy, Josep Maria
dc.creator Quandt Rodríguez, Milan
dc.date 2018-10-09T15:14:25Z
dc.date 2018-10-09T15:14:25Z
dc.date 2018-06
dc.date.accessioned 2024-12-16T10:26:50Z
dc.date.available 2024-12-16T10:26:50Z
dc.identifier http://hdl.handle.net/2445/125200
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/21564
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Josep Maria Paredes Poy
dc.description We apply the Van der Laan model to the microquasar GRS 1915+105 and extract parameters that fit the radio emission curves best. We obtain values for the energy spectral index in the range of p ∼ 0:7 - 0:8 for the fit, which largely disagree with the ones predicted by the model, about p ∼ 0:1. This results suggest that to model synchrotron radio emission of X-ray binaries we need to take into account events such as continuous injection and energy losses, as well as a jet-like geometry rather than a spherically symmetric one
dc.format 5 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Quandt, 2018
dc.rights http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights info:eu-repo/semantics/openAccess
dc.source Treballs Finals de Grau (TFG) - Física
dc.subject Quàsars
dc.subject Radioastronomia
dc.subject Treballs de fi de grau
dc.subject Quasars
dc.subject Radio astronomy
dc.subject Bachelor's theses
dc.title The Van der Laan extragalactic emission model applied to GRS 1915+105
dc.type info:eu-repo/semantics/bachelorThesis


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