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

Published online by Cambridge University Press:  21 October 2010

E. M. Reynoso ,
H. L. Gomez  and
L. Dunne
E. M. Reynoso
Affiliation:
IAFE (CONICET-UBA) and Physics Dept. (FCEyN, UBA), Buenos Aires, Argentina
H. L. Gomez
Affiliation:
School of Physics and Astronomy, Cardiff University, The Parade, Wales, UK
L. Dunne
Affiliation:
School of Physics and Astronomy, University of Nottingham, UK
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Abstract

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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

dustsupernova remnantsindividual: Kepler's SNRsubmillimetre
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

References

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