Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-11T13:51:36.049Z Has data issue: false hasContentIssue false
  • English
  • Français

The Dust Content and Temperature Distribution of Galaxies in The Local Universe

Published online by Cambridge University Press:  01 August 2006

S. Falony ,
M. Baes ,
J. I. Davies  and
C. Vlahakis
S. Falony
Affiliation:
Universiteit Gent, Belgium, email: [email protected]
M. Baes
Affiliation:
Universiteit Gent, Belgium, email: [email protected]
J. I. Davies
Affiliation:
Cardiff University, UK
C. Vlahakis
Affiliation:
Bonn University, Germany
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 measured the SCUBA fluxes of a sample of Seyfert 1, Seyfert 2, starburst and normal disc galaxies, taken from the Extended 12 Micron Galaxy Sample. From these data, we determine the entire dust content and temperature distribution of galaxies of different classes through a Planckian inversion technique.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 95
Copyright
Copyright © International Astronomical Union 2007