Speaker
JIAN LI
(Institute of Space Sciences (CSIC-IEEC))
Description
We present the results of the analysis of 8 years of Fermi-LAT data of the pulsar/pulsar wind nebula complex PSRJ0205+6449/3C 58. Using a contemporaneous ephemeris, we carried out a detailed analysis of PSRJ0205+6449 both during its off-peak and on-peak phase intervals. 3C 58 is significantly detected during the off-peak phase interval. Hints for a possible flare from 3C 58 are identified. We show that the spectral energy distribution at high energies is the same disregarding the phases considered, and thus that this part of the spectrum is most likely dominated by the nebula radiation. We present results of theoretical models of the nebula and the magnetospheric emission that confirm this
interpretation.
Primary author
JIAN LI
(Institute of Space Sciences (CSIC-IEEC))
Co-author
Diego Torres
(ICREA & Institute of Space Sciences)
