Paredes i Poy, Josep MariaLópez Ramiro, Èric2016-03-092016-03-092016-01https://hdl.handle.net/2445/96320Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: Josep Maria Paredes PoyWe 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+1055 p.application/pdfengcc-by-nc-nd (c) López, 2016http://creativecommons.org/licenses/by-nc-nd/3.0/es/Radiació sincrotrònicaEstels binaris de raigs XTreballs de fi de grauSynchrotron radiationX-ray binariesBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess