SN1987A at 18 Years: Ejecta-Ring Interaction

Details SN1987A at 18 Years: Ejecta-Ring Interaction SN1987A at 18 Years: Ejecta-Ring Interaction

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..924..383d&link_type=abstract

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 383-388

Physics

Supernovae, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus

Scientific paper

After 18 years the outer parts of the ejecta of SN1987A are interacting
with the inner ring. This ejecta-ring interaction is the source of most
of the activity associated with the supernova. The physical effects are
detectable at all accessible wavelengths. Some of these are described
with particular focus on IR radiation associated with dust.

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