Supernova 1987A: A young supernova remnant in an aspherical progenitor wind

(2) ATNF); A. K. Tzioumis (2); B. M. Gaensler (1); J. E. Reynolds (2); L. Staveley-Smith (2); M. J. Kesteven (2) ((1) MIT; R. N. Manchester (2); V. Wheaton (2)

arxiv: astro-ph/9909396 · v1 · submitted 1999-09-23 · 🌌 astro-ph

Supernova 1987A: A young supernova remnant in an aspherical progenitor wind

B. M. Gaensler (1) , R. N. Manchester (2) , L. Staveley-Smith (2) , V. Wheaton (2) , A. K. Tzioumis (2) , J. E. Reynolds (2) , M. J. Kesteven (2) ((1) MIT , (2) ATNF) This is my paper

classification 🌌 astro-ph

keywords supernovainteractionprogenitorremnantwindasphericalaxisymmetricbeen

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The interaction between the ejecta from Supernova 1987A and surrounding material is producing steadily brightening radio and X-ray emission. The new-born supernova remnant has been significantly decelerated by this interaction, while its morphology reflects the axisymmetric nature of the progenitor wind.

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Supernova 1987A: A young supernova remnant in an aspherical progenitor wind

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