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DC Field | Value | Language |
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dc.contributor.advisor | Paredes i Poy, Josep Maria | - |
dc.contributor.author | López Ramiro, Èric | - |
dc.date.accessioned | 2016-03-09T16:43:56Z | - |
dc.date.available | 2016-03-09T16:43:56Z | - |
dc.date.issued | 2016-01 | - |
dc.identifier.uri | http://hdl.handle.net/2445/96320 | - |
dc.description | Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: Josep Maria Paredes Poy | ca |
dc.description.abstract | We present the model proposed by van der Laan (1966) to describe the evolution of the flux emitted by a spherical cloud in adiabatic expansion whose electrons follow a power law N(E) / E−p. The model is tested in order to apply it to the light curves corresponding to the data obtained on May 15, 1997 from observation on the X-ray binary star system GRS 1915+105 | ca |
dc.format.extent | 5 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | ca |
dc.rights | cc-by-nc-nd (c) López, 2016 | - |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | - |
dc.source | Treballs Finals de Grau (TFG) - Física | - |
dc.subject.classification | Radiació sincrotrònica | cat |
dc.subject.classification | Estels binaris de raigs X | cat |
dc.subject.classification | Treballs de fi de grau | cat |
dc.subject.other | Synchrotron radiation | eng |
dc.subject.other | X-ray binaries | eng |
dc.subject.other | Bachelor's theses | eng |
dc.title | Synchrotron emission in stellar systems: the case of GRS 1915+105 | eng |
dc.type | info:eu-repo/semantics/bachelorThesis | ca |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca |
Appears in Collections: | Treballs Finals de Grau (TFG) - Física |
Files in This Item:
File | Description | Size | Format | |
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TFG_Fis_Lopez_Ramiro_Eric.pdf | 2.48 MB | Adobe PDF | View/Open |
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