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- W4385681530 abstract "Supernovae (SN) explosions are thought to be an important source of dust in galaxies. At the same time strong shocks from SNe are known as an efficient mechanism of dust destruction via thermal and kinetic sputtering. A critically important question of how these two hypotheses of SNe activity control the dust budget in galaxies is still not quite clearly understood. In this paper we address this question within 3D multi-fluid hydrodynamical simulations, treating separately the SNe injected dust and the dust pre-exicted in ambient interstellar gas. We focus primarily on how the injected and pre-existed dust are destroyed by shock waves and the hot gas in the SN bubble depending of the density of ambient gas. Within our model we estimate an upper limit of the SN-produced dust mass which can be supplied into interstellar medium. For a SN progenitor mass of 30 $M_odot$ and the ejected dust mass $M_d=1~M_odot$ we constrain the dust mass that can delivered into the ISM as $geq 0.13~M_odot$ provided the injected dust particles are large $ageq 0.1~mu$m." @default.
- W4385681530 created "2023-08-09" @default.
- W4385681530 creator A5074432040 @default.
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- W4385681530 date "2023-08-06" @default.
- W4385681530 modified "2023-10-16" @default.
- W4385681530 title "Dust evolution in a supernova interacting with the ISM" @default.
- W4385681530 doi "https://doi.org/10.48550/arxiv.2308.03106" @default.
- W4385681530 hasPublicationYear "2023" @default.
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