Dust production in supernovae: the case of Kepler's SNR

Details Dust production in supernovae: the case of Kepler's SNR Dust production in supernovae: the case of Kepler's SNR

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..425r&link_type=abstract

Highlights of Astronomy, Volume 15, p. 425-425

Astronomy and Astrophysics

Astronomy

Dust, Supernova Remnants, Individual: Kepler'S Snr, Submillimetre

Scientific paper

We compare the submillimetre (submm) emission with the Hi and CO
distribution towards Kepler's supernova remnant (SNR), and conclude that
0.1 to 1.2 M&sun; of dust originates from Kepler. Such rates
are sufficient to explain the origin of dust in high redshift galaxies.

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