The mass of dust in Cassiopeia A

Details The mass of dust in Cassiopeia A The mass of dust in Cassiopeia A

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..439w&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Computer Science

Supernovae: Cassiopeia A, Ism: Sub-Mm Dust Emission, Radio Lines

Scientific paper

Recent observations of sub-millimeter continuum emission toward supernova remnants (SNR) have raised the question of whether such emission is caused by dust within the SNR and thus produced by the supernova itself or along the line-of-sight. Here we make a comparison of the image of sub-mm emission from dust with the integrated J = 1-0 line emission from interstellar 13CO toward the SNR Cassiopeia A. Our goal in this comparison is to collect hard evidence which tests whether dust at high redshifts can be produced in Supernovae.

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