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

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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.
4 pages, 2 embedded EPS figures, uses newpasp.sty. To appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures,'' ASP Conference Series, J.H. Kastner, N. Soker, & S.A. Rappaport, eds

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http://salesiana.dossiersoluciones.com/handle/123456789/14842

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9909396
 http://arxiv.org/abs/astro-ph/9909396

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arXiv