XMM-Newton observations of HESS J1813-178 reveal a composite Supernova remnant

S. Funk, J. Vink

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

We present X-ray and 12CO(J=1-0) observations of the very-high-energy (VHE) γ-ray source HESS J1813-178 with the aim of understanding the origin of the γ-ray emission. We discuss the scenario in which the γ-rays originate in the shell of the SNR, and that in which they originate in the central object, in terms of a time-dependent one-zone leptonic model. We demonstrate, that in order to connect the core X-ray emission to the VHE γ-ray emission electrons have to be accelerated to energies of at least 1 PeV.
Original languageUndefined/Unknown
Pages (from-to)249-257
Number of pages9
JournalAstronomy and Astrophysics
Volume470
Issue number1
Publication statusPublished - 2007

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