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

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.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.identifier.uri	https://hdl.handle.net/2445/96320
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) López, 2016
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
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

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