Title of article
Dust production in supernovae: the case of Kepler’s SNR
Author/Authors
E. M. Reynoso، نويسنده , , H. L. Gomez، نويسنده , , L. Dunne، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2009
Pages
1
From page
425
To page
425
Abstract
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_ of dust originates from Kepler. Such rates are sufficient to explain the origin of dust in high redshift galaxies.
Keywords
Supernova remnants , individual: Kepler’s SNR , submillimetre , dust
Journal title
Proceedings of the International Astronomical Union
Serial Year
2009
Journal title
Proceedings of the International Astronomical Union
Record number
674754
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