Líneas ciclo trónicas en el espectro de rayos y pulsado

  • Jorge Paez Grupo de Astrofísica, Escuela de Física, Universidad de Costa Rica
  • L. Semionova N. Departamento de Física, Universidad Nacional


If the magnetic Bremsstrahlung process is responsable for the lines observes in the spectra of two y-ray bursts, GB880205 and GB870303 detected by the spectrometer of the GINGA satelite, then the fundamental and primary harmonics (transition between the excited Landau levels N=2,1 to the ground-state N´=0) may be identified as the cause of those features detected in those y-ray bursts. We use the transition rate for this process in order to prove our asseveration. We suppose that this process is occurring under the presence of an external magnetic field of order 2*10 12 Gauss. The numerical results for the energy average of the emitted photons are: 22.41 Kev and 43.86 Kev. These energies correspond to the fundamental and primary harmonics transition respectively.

Subjet headings: y-rays- magnetic fields- radiation mechanisms.

How to Cite
Paez, J., & Semionova N., L. (1989). Líneas ciclo trónicas en el espectro de rayos y pulsado. Uniciencia, 6(1-2), 97-107. Retrieved from https://www.revistas.una.ac.cr/index.php/uniciencia/article/view/5428
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