We present observations of the young supernova remnant (SNR) RXJ1713.7-3946 with the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with the SNR. The source is extended with a best-fit extension of 055 ± 004 matching the size of the non-thermal X-ray and TeV gamma-ray emission from the remnant. The positional coincidence and the matching extended emission allow us to identify the LAT source with SNR RXJ1713.7-3946. The spectrum of the source can be described by a very hard power law with a photon index of Γ = 1.5 0.1 that coincides in normalization with the steeper H.E.S.S.-detected gamma-ray spectrum at higher energies. The broadband gamma-ray emission is consistent with a leptonic origin as the dominant mechanism for the gamma-ray emission.

Observations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope / Abdo, A.a., Ackermann, M., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Barbiellini, G., Baring, M.g., Bastieri, D., Bellazzini, R., Berenji, B., Blandford, R.d., Bloom, E.d., Bonamente, E., Borgland, A.w., Bouvier, A., Brandt, T.j., Bregeon, J., Brigida, M., Bruel, P., et al.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 734:1(2011). [10.1088/0004-637X/734/1/28]

Observations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope

FAVUZZI, Cecilia;GIGLIETTO, Nicola;
2011

Abstract

We present observations of the young supernova remnant (SNR) RXJ1713.7-3946 with the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with the SNR. The source is extended with a best-fit extension of 055 ± 004 matching the size of the non-thermal X-ray and TeV gamma-ray emission from the remnant. The positional coincidence and the matching extended emission allow us to identify the LAT source with SNR RXJ1713.7-3946. The spectrum of the source can be described by a very hard power law with a photon index of Γ = 1.5 0.1 that coincides in normalization with the steeper H.E.S.S.-detected gamma-ray spectrum at higher energies. The broadband gamma-ray emission is consistent with a leptonic origin as the dominant mechanism for the gamma-ray emission.
2011
Observations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope / Abdo, A.a., Ackermann, M., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Barbiellini, G., Baring, M.g., Bastieri, D., Bellazzini, R., Berenji, B., Blandford, R.d., Bloom, E.d., Bonamente, E., Borgland, A.w., Bouvier, A., Brandt, T.j., Bregeon, J., Brigida, M., Bruel, P., et al.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 734:1(2011). [10.1088/0004-637X/734/1/28]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/51983
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