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- W2149804889 abstract "We present a numerical simulation carried out in order to explain the complex morphology of the supernova remnant (SNR) 3C 400.2. Numerical simulations were done employing the new yguaz u-a code (Raga et al. 2000). In the radio continuum, this remnant seems to be formed by two shells, which are par- tially overlapping (Dubner et al. 1994). Taking into account observational evidence such as a previous HI study (Giacani et al. 1998), we nd that an adequate model for describing the morphology of the SNR 3C 400.2 is obtained by assuming that a single supernova (SN) explosion took place in a dense medium and close to an interface separating this medium from a lower density region. Besides, we also present a new deeper CCD H image mosaic of the north{west region of this SNR, which is composed of three single images. From the numerical results, we generated H emission maps, obtaining a good agreement with the observations." @default.
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- W2149804889 date "2001-10-01" @default.
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- W2149804889 title "A single explosion model for the supernova remnant 3C 400.2" @default.
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- W2149804889 doi "https://doi.org/10.1051/0004-6361:20011116" @default.
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