High-resolution radio imaging of young supernovae
classification
🌌 astro-ph
keywords
radiosupernovaevlbiyoungdirectlyexpandinggiveshere
read the original abstract
The high resolution obtained through the use of VLBI gives an unique opportunity to directly observe the interaction of an expanding radio supernova with its surrounding medium. We present here results from our VLBI observations of the young supernovae SN 1979C, SN 1986J, and SN 2001gd.
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.