Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-23T18:50:52.196Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Dunne, L. et al. , 2009, MNRAS, 394, 1307Google Scholar
Gomez, H. L., Dunne, L., Ivison, R. J., Reynoso, E. M., Thompson, M. A., Sibthorpe, B., Eales, S. A., DeLaney, T. M., Maddox, S., & Isaak, K. 2009, MNRAS 397, 1621Google Scholar
Krause, O., et al. , 2004, Nature, 432, 596Google Scholar
Morgan, H. L., Dunne, L., Eales, S., Ivison, R. J., & Edmunds, M. G., 2003, ApJ, 597, L33Google Scholar
Rho, J., et al. , 2008, ApJ, 673, 271Google Scholar