Interstellar Dust in the Large Magellanic Cloud
Abstract
New IUE observations confirm the differences between the galactic and LMC ultraviolet extinction curves and show some evidence for variations within the LMC. Visual and infrared photometry and polarimetry show that the anomalous properties of the LMC dust do not extend to longer wavelengths.
- Publication:
-
Structure and Evolution of the Magellanic Clouds
- Pub Date:
- September 1984
- DOI:
- 10.1017/S0074180900040602
- Bibcode:
- 1984IAUS..108..403C