A Morphological Criterion for Distinguishing Between Supernova Remnants and HII Regions

Details A Morphological Criterion for Distinguishing Between Supernova Remnants and HII Regions A Morphological Criterion for Distinguishing Between Supernova Remnants and HII Regions

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..358i&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO.2/SEP15, P. 358, 1990

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A variant of the vector discriminant pattern recognition technique is applied to UK Schmidt telescope images of nebulae in the Large Magellanic Cloud. A criterion is thereby obtained which may be applied generally to distinguish between supernova remnants (SNRs) and H II regions from their optical images. Furthermore, two nebulae previously identified as H II regions are now interpreted as SNRs.

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