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A new method to determine the relation between dust mass and submm luminosity

James, A., Dunne, Loretta, Eales, Stephen Anthony ORCID: https://orcid.org/0000-0002-7394-426X and Edmunds, Michael Geoffrey 2003. A new method to determine the relation between dust mass and submm luminosity. Presented at: Galaxy evolution : theory and observations, Cozumel, Quintana Roo, México, 8 - 12 April 2002. Published in: Avila-Reese, Vladimir, Firmani, Claudio, Frenk, Carlos S. and Allen, Christine eds. Galaxy evolution : theory and observations : Cozumel, Quintana Roo, México, abril 8-12, 2002. Revista mexicana de astronomía y astrofisíca (RevMexAA)- Serie de Conferencias (17) Cozumel, Mexico: Instituto de Astronomía, Universidad Nacional Autónoma de México, p. 269.

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Abstract

Using a new technique we have determined a value for the dust mass absorption coefficient at 850 mu m. We find kappa_{{850}}() = 0.07+/-0.02m2kg-1

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: Instituto de Astronomía, Universidad Nacional Autónoma de México
ISBN: 9703206093
Related URLs:
Last Modified: 24 Oct 2022 11:30
URI: https://orca.cardiff.ac.uk/id/eprint/48374

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