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

Reynoso, E. M., Gomez, Haley Louise ORCID: https://orcid.org/0000-0003-3398-0052 and Dunne, L. 2009. Dust production in supernovae: the case of Kepler's SNR [Abstract]. Proceedings of the International Astronomical Union 5 (H15) , p. 425. 10.1017/S1743921310010094

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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.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Uncontrolled Keywords:	dust; supernova remnants; individual: Kepler's SNR; submillimetre
Additional Information:	Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/1743-9213/ (accessed 21/02/2014).
Publisher:	Cambridge University Press
ISSN:	1743-9213
Date of First Compliant Deposit:	30 March 2016
Last Modified:	03 May 2023 19:15
URI:	https://orca.cardiff.ac.uk/id/eprint/22244

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