Computer Science
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205..366p&link_type=abstract
Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at
Computer Science
3
Scientific paper
This is a review current observations of radio supernovae & supernova remnants in external galaxies. The advantages of studying samples of supernova remnants in external galaxies will be discussed, and recent expansion velocity measurements described. A summary of how the remnants can be used to infer starformation rates in these galaxies will be given, as will the use of these remnants to probe the interstellar medium of starburst galaxies on parsec scales. Recent widefield EVN and Global VLBI measurements of remnants in the nearby starburst in M82 will be described in detail, and the similarity between the strongest compact source in M82 and the objects recently discovered in Arp220 will be noted. The sensitivity limitations of this work will be discussed and the prospects for studies of more distant objects using Square Kilometer Array considered.
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