A CR-HYDRO-NEI MODEL OF MULTI-WAVELENGTH EMISSION FROM THE VELA JR. SUPERNOVA REMNANT (SNR RX J0852.0–4622)

• Lee, Shiu-Hang

• Slane, Patrick O.

• Ellison, Donald C.

• Nagataki, Shigehiro

• Patnaude, Daniel J.

抄録

Based largely on energy budget considerations and the observed cosmic-ray (CR) ionic composition, supernova remnant (SNR) blast waves are the most likely sources of CR ions with energies at least up to the "knee" near 10^[15] eV. Shocks in young shell-type TeV-bright SNRs are surely producing TeV particles, but the emission could be dominated by ions producing π^0-decay emission or electrons producing inverse Compton gamma rays. Unambiguously identifying the GeV-TeV emission process in a particular SNR will not only help pin down the origin of CRs, it will also add significantly to our understanding of the diffusive shock acceleration (DSA) mechanism and improve our understanding of supernovae and the impact SNRs have on the circumstellar medium. In this study, we investigate the Vela Jr. SNR, an example of TeV-bright non-thermal SNRs. We perform hydrodynamic simulations coupled with nonlinear DSA and non-equilibrium ionization near the forward shock to confront currently available multi-wavelength data. We find, with an analysis similar to that used earlier for SNR RX J1713.7–3946, that self-consistently modeling the thermal X-ray line emission with the non-thermal continuum in our one-dimensional model strongly constrains the fitting parameters, and this leads convincingly to a leptonic origin for the GeV-TeV emission for Vela Jr. This conclusion is further supported by applying additional constraints from observation, including the radial brightness profiles of the SNR shell in TeV gamma rays, and the spatial variation of the X-ray synchrotron spectral index. We will discuss implications of our models on future observations by the next-generation telescopes.

収録刊行物

• The Astrophysical Journal

  The Astrophysical Journal 767 (1), 2013-03-21

  IOP Publishing

キーワード

• acceleration of particles
• cosmic rays
• ISM
• supernova remnants
• shock waves

詳細情報

• CRID: 1050001335767351552
• NII論文ID: 120005244419
• NII書誌ID: AA00553242
• ISSN: 0004637X
• HANDLE: 2433/173353
• 本文言語コード: en
• 資料種別: journal article
• データソース種別:
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  • CiNii Articles