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.

Full text not available from this repository.

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:	http://www.astroscu.unam.mx/rmaa/RMxAC.....
Last Modified:	24 Oct 2022 11:30
URI:	https://orca.cardiff.ac.uk/id/eprint/48374

Citation Data

Cited 1 time in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item