Taking advantage of 10 years of Fermi-LAT data, we perform a new and deep analysis of the pulsar wind nebula (PWN) HESS J1825-137. We present the results of the spectral analysis and of the first energy-resolved morphological study of the PWN HESS J1825-137 from 1 GeV to 1 TeV. This PWN is an archetypal system making it a perfect laboratory for studying particle transport mechanisms. Combining this analysis with recent H.E.S.S. results enables a more complete picture of the nebula to emerge.
Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by the Fermi-LAT / Principe, G; Mitchell, ; Hinton, ; J., search by orcid; Parson, ; Caroff, ; Hahn, ; Funk,. - (2019), pp. ---. ( 36th International Cosmic Ray Conference Madison July 2019).
Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by the Fermi-LAT
PRINCIPE G;
2019-01-01
Abstract
Taking advantage of 10 years of Fermi-LAT data, we perform a new and deep analysis of the pulsar wind nebula (PWN) HESS J1825-137. We present the results of the spectral analysis and of the first energy-resolved morphological study of the PWN HESS J1825-137 from 1 GeV to 1 TeV. This PWN is an archetypal system making it a perfect laboratory for studying particle transport mechanisms. Combining this analysis with recent H.E.S.S. results enables a more complete picture of the nebula to emerge.Pubblicazioni consigliate
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