Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2025-01-06T03:19:29.134Z Has data issue: false hasContentIssue false
  • English
  • Français

Large scale distribution of gas, dust and stars deduced from observations from the UV to the IR

Published online by Cambridge University Press:  19 July 2016

J. Koornneef
J. Koornneef*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

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We introduce an as yet unpublished set of OAO-II observations of stellar associations in the Large Magellanic Cloud (LMC). Cross-correlation of the photometric characteristics of these fields with the infrared fluxes at these same positions obtained by the IRAS satellite provides information on the local stellar population, the amounts of interstellar extinction and thermal dust emission.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 69 - 70
Copyright
Copyright © Kluwer 1991