Synchrotron emission in stellar systems: the case of GRS 1915+105

dc.contributor	Paredes i Poy, Josep Maria
dc.creator	López Ramiro, Èric
dc.date	2016-03-09T16:43:56Z
dc.date	2016-03-09T16:43:56Z
dc.date	2016-01
dc.date.accessioned	2024-12-16T10:22:11Z
dc.date.available	2024-12-16T10:22:11Z
dc.identifier	http://hdl.handle.net/2445/96320
dc.identifier.uri	http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/13909
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: Josep Maria Paredes Poy
dc.description	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
dc.format	5 p.
dc.format	application/pdf
dc.language	eng
dc.rights	cc-by-nc-nd (c) López, 2016
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	Radiació sincrotrònica
dc.subject	Estels binaris de raigs X
dc.subject	Treballs de fi de grau
dc.subject	Synchrotron radiation
dc.subject	X-ray binaries
dc.subject	Bachelor's theses
dc.title	Synchrotron emission in stellar systems: the case of GRS 1915+105
dc.type	info:eu-repo/semantics/bachelorThesis

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