Young Supernova Remnants in the Magellanic Clouds
arXiv:astro-ph/0102377 · doi:10.1063/1.1377130
Abstract
There are a half-dozen or so young supernova remnants in the Magellanic Clouds that display one or more of the following characteristics: high velocity (>1000 km/s) emission, enhanced metallicity, or a rapidly rotating pulsar. I summarize the current state of knowledge of these remnants and present some recent results mostly from the new X-ray astronomy satellites.
10 pages, including 8 postscript figs, LaTeX. To appear in the Proceedings of the 11th Annual October Maryland Astrophysics Conference ``Young Supernova Remnants''
Cited by in corpus (4)
- High resolution spectroscopy and emission line imaging of DEM L 71 with XMM-Newton
- A Deep Chandra Observation of the Oxygen-Rich Supernova Remnant 0540-69.3 in the Large Magellanic Cloud
- The Discovery of a Spatially-Resolved Supernova Remnant in M31 with Chandra
- X-ray/Optical/Radio Observations of a Resolved Supernova Remnant in NGC 6822