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Dust production in supernovae: the case of Kepler's SNR
Published online by Cambridge University Press: 21 October 2010
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 425
- Copyright
- Copyright © International Astronomical Union 2010