# name
Synchrotron emission in supernova remanants

# metadata.dc.description[].value
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Josep Maria Paredes Poy

# metadata.dc.description.abstract[].value
We have studied the spectrum of the 3C 391 supernova remnant by means of the integrated density flux. The fit of the data was made considering that the synchrotron emission is affected by free-free absorption at low frequencies. The value we obtained for the optical depth at 74 MHz is τ74 = 1.06±0.09, showing that there is strong absorption in that region. The study from which this data was obtained, indicate that the medium responsible for the absorption could be a thermal ionized gas linked to the SNR itself

# metadata.dc.title[].value
Synchrotron emission in supernova remanants