Physics
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aujph..32..113l&link_type=abstract
(Joint Australia-USSR-USA Symposium on Pulsars and Supernova Remnants, Sydney, Australia, Apr. 1978.) Australian Journal of Phys
Physics
11
Gas Expansion, H Alpha Line, Radial Velocity, Supernova Remnants, Flow Velocity, High Speed
Scientific paper
Interferometric H-alpha observations have been made of faint filaments
and high-velocity diffuse gas in the supernova remnants IC 443 and VRO
42.05.01. In both cases the implied expansion velocities are
substantially higher than those obtained from the velocities of the
bright filaments.
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