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

B. M. Gaensler·R. N. Manchester·L. Staveley-Smith·V. Wheaton·A. K. Tzioumis·J. E. Reynolds·M. J. Kesteven
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Abstract

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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B. M. Gaensler, R. N. Manchester, L. Staveley-Smith, V. Wheaton, A. K. Tzioumis, J. E. Reynolds, M. J. Kesteven. 1999-09-23. Supernova 1987A: A young supernova remnant in an aspherical progenitor wind. https://arxiv.org/abs/astro-ph/9909396

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