Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-12T21:12:15.173Z Has data issue: false hasContentIssue false
  • English
  • Français

The Herschel view on the dust properties of the Large Magellanic Cloud

Published online by Cambridge University Press:  21 March 2013

Frédéric Galliano
Frédéric Galliano*
Affiliation:
AIM, L'Orme des Merisiers, CEA/Saclay, 91191 Gif-sur-Yvette, France
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.

I summarize a recent study scrutinizing the various sources of uncertainties in estimating the dust mass of a galaxy. These effects are demonstrated on the Herschel observations of the Large Magellanic Cloud.

Keywords

galaxies: ISM — Magellanic Clouds — dust — ISM: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 285
Copyright
Copyright © International Astronomical Union 2013

References

Galliano, F., Hony, S., Bernard, J.-P., Bot, C., Madden, S. C.et al. 2011, A&A, 536, A88Google Scholar