超新星 1987A：一种非球对称 progenitor 风中的年轻超新星残余
天体物理学
2007-05-23 v1
摘要
超新星 1987A 的 ejecta 与周围物质的相互作用正在产生持续变亮的射电和 X 射线辐射。新生的超新星残余因与这种相互作用而显著减速，而其形态反映了 progenitor 风的轴对称性质。
引用
@article{arxiv.astro-ph/9909396,
title = {Supernova 1987A: A young supernova remnant in an aspherical progenitor wind},
author = {B. M. Gaensler and R. N. Manchester and L. Staveley-Smith and V. Wheaton and A. K. Tzioumis and J. E. Reynolds and M. J. Kesteven},
journal= {arXiv preprint arXiv:astro-ph/9909396},
year = {2007}
}
备注
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