HI Study of Southern Galactic Supernova Remnants

Details HI Study of Southern Galactic Supernova Remnants HI Study of Southern Galactic Supernova Remnants

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..317...41k&link_type=abstract

Milky Way Surveys: The Structure and Evolution of our Galaxy, Proceedings of ASP Conference #317. The 5th Boston University Ast

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We searched HI 21-cm line emission from shocked atomic gas associated with southern supernova remnants (SNRs) using the Southern Galactic Plane Survey. Among 97 sources, we detected 10 SNRs that have been associated with high-velocity HI gas, most of which are quite possibly the gas accelerated by the SN blast wave. We also detected about 5 SNRs that possibly have been associated with HI shells. These sources show an excess HI emission significantly brighter than the surrounding region over a wide (>10 km s-1) velocity interval.

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