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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/96320
Synchrotron emission in stellar systems: the case of GRS 1915+105
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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
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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: Josep Maria Paredes Poy
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LÓPEZ RAMIRO, Èric. Synchrotron emission in stellar systems: the case of GRS 1915+105. [consulted: 10 of June of 2026]. Available at: https://hdl.handle.net/2445/96320