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- W130412509 abstract "The shock wave of shell supernova remnant (SNR) offers the unique opportunity to detect directly the structures of the interstellar medium, both at large and small scale. Unfortunately, the several physical effects at work in the interaction between the shock and the medium, along with the superposition effects along a given light of sight, require detailed modeling and high resolution observations of the systems in order to understand its physical behavior At the Osservatorio Astronomico di Palermo, we have started a longterm project which will lead, for the first time, to a self-consistent methodological approach for comparison of new accurate numerical models and high resolution multi-wavelength observations. In this poster, we introduce the observation we have already analyzed,while in the talk of S. Orlando the new numerical models we have developed are presented" @default.
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- W130412509 date "2006-01-01" @default.
- W130412509 modified "2023-09-27" @default.
- W130412509 title "X-raying the interstellar medium: the study of SNR shells at the OAPa" @default.
- W130412509 hasPublicationYear "2006" @default.
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