1999/09/23 by B. M. Gaensler, Gaensler, B. M., R. N. Manchester +13
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9909396
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
arxiv created 1999/09/23 · openalex publication_date 1999/09/23 · arxiv updated 2009/12/01 · openalex created_date 2019/12/05 · openalex updated_date 2026/07/28
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.