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• W4313856931 endingPage "5372" @default.
• W4313856931 startingPage "5358" @default.
• W4313856931 abstract "ABSTRACT Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide insights into the evolutionary history of the progenitor star. But while some SNRs are spherical, as expected from a point-like explosion expanding into a roughly uniform medium, many others exhibit complex non-spherical morphologies that are often not easily explained. In this work, we use 3D magnetohydrodynamic simulations to show that rectangular and jet-like morphologies can be explained by supernovae (SNe), either type Ia or type II, expanding within anisotropic, bipolar stellar wind bubbles driven by the progenitor star. The stellar wind has an anisotropic density distribution, which channels the SN ejecta differently depending on the anisotropy characteristics. We compute synthetic thermal (X-ray) and non-thermal (synchrotron) emission maps from our numerical simulations to compare with observations. We find rectangular morphologies are generated when the stellar wind has a high-mass loss rate and forms a dense, narrow disc at the equatorial region. Instead, a jet-like or ear-like morphology is obtained when the stellar wind develops a wide, dense disc. Stellar winds with low mass-loss rates do not strongly influence the SNR morphology. Finally, our synthetic synchrotron and X-ray maps for the high mass-loss rate case qualitatively agree with the observations of the SNRs G332.5-5.6 and G290.1-0.8." @default.
• W4313856931 created "2023-01-10" @default.
• W4313856931 creator A5002273758 @default.
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• W4313856931 date "2023-01-09" @default.
• W4313856931 modified "2023-10-15" @default.
• W4313856931 title "The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially confined progenitor stellar winds" @default.
• W4313856931 cites W107140549 @default.
• W4313856931 cites W1882205232 @default.
• W4313856931 cites W1948604961 @default.
• W4313856931 cites W1973017976 @default.
• W4313856931 cites W1985970073 @default.
• W4313856931 cites W1989432205 @default.
• W4313856931 cites W1991860486 @default.
• W4313856931 cites W2001289103 @default.
• W4313856931 cites W2002974377 @default.
• W4313856931 cites W2006726020 @default.
• W4313856931 cites W2013997547 @default.
• W4313856931 cites W2021336476 @default.
• W4313856931 cites W2047460464 @default.
• W4313856931 cites W2048474698 @default.
• W4313856931 cites W2051120619 @default.
• W4313856931 cites W2059049415 @default.
• W4313856931 cites W2065892679 @default.
• W4313856931 cites W2065931799 @default.
• W4313856931 cites W2073342600 @default.
• W4313856931 cites W2077136186 @default.
• W4313856931 cites W2077310516 @default.
• W4313856931 cites W2087069688 @default.
• W4313856931 cites W2088776898 @default.
• W4313856931 cites W2091166540 @default.
• W4313856931 cites W2096177980 @default.
• W4313856931 cites W2096911128 @default.
• W4313856931 cites W2103622259 @default.
• W4313856931 cites W2110916902 @default.
• W4313856931 cites W2125253967 @default.
• W4313856931 cites W2139741136 @default.
• W4313856931 cites W2140888726 @default.
• W4313856931 cites W2157990947 @default.
• W4313856931 cites W2163314526 @default.
• W4313856931 cites W2168652991 @default.
• W4313856931 cites W2293704115 @default.
• W4313856931 cites W2511857982 @default.
• W4313856931 cites W2529229450 @default.
• W4313856931 cites W2782865078 @default.
• W4313856931 cites W2789572870 @default.
• W4313856931 cites W2798740635 @default.
• W4313856931 cites W2807558337 @default.
• W4313856931 cites W2962785036 @default.
• W4313856931 cites W2978929356 @default.
• W4313856931 cites W3002265977 @default.
• W4313856931 cites W3007543527 @default.
• W4313856931 cites W3023103226 @default.
• W4313856931 cites W3025239494 @default.
• W4313856931 cites W3033722482 @default.
• W4313856931 cites W3087500512 @default.
• W4313856931 cites W3094898175 @default.
• W4313856931 cites W3098009603 @default.
• W4313856931 cites W3098663361 @default.
• W4313856931 cites W3098763385 @default.
• W4313856931 cites W3100045092 @default.
• W4313856931 cites W3100798857 @default.
• W4313856931 cites W3102199807 @default.
• W4313856931 cites W3102388023 @default.
• W4313856931 cites W3102893717 @default.
• W4313856931 cites W3103551677 @default.
• W4313856931 cites W3103716838 @default.
• W4313856931 cites W3104101109 @default.
• W4313856931 cites W3104137987 @default.
• W4313856931 cites W3104282706 @default.
• W4313856931 cites W3106398819 @default.
• W4313856931 cites W3117200161 @default.
• W4313856931 cites W3126479898 @default.
• W4313856931 cites W3127459630 @default.
• W4313856931 cites W3141260686 @default.
• W4313856931 cites W3179952852 @default.
• W4313856931 cites W3207726085 @default.
• W4313856931 cites W3210826688 @default.
• W4313856931 cites W3212737794 @default.
• W4313856931 cites W4211072419 @default.
• W4313856931 cites W4213012707 @default.
• W4313856931 cites W4220663557 @default.
• W4313856931 cites W4280535540 @default.
• W4313856931 cites W4283749604 @default.
• W4313856931 cites W4283761616 @default.
• W4313856931 cites W4288076647 @default.
• W4313856931 cites W4288079654 @default.
• W4313856931 cites W4292764441 @default.
• W4313856931 cites W4301366182 @default.
• W4313856931 doi "https://doi.org/10.1093/mnras/stad039" @default.
• W4313856931 hasPublicationYear "2023" @default.
• W4313856931 type Work @default.

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