Young Supernova Remnants in the Magellanic Clouds
classification
🌌 astro-ph
keywords
remnantscloudsmagellanicsupernovayoungastronomycharacteristicscurrent
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.