Young Supernova Remnants in the Magellanic Clouds

Details Young Supernova Remnants in the Magellanic Clouds Young Supernova Remnants in the Magellanic Clouds

2001-02-21

arxiv.org/abs/astro-ph/0102377v1

Astronomy and Astrophysics

Astrophysics

10 pages, including 8 postscript figs, LaTeX. To appear in the Proceedings of the 11th Annual October Maryland Astrophysics Co

Scientific paper

10.1063/1.1377130

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.

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