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Dust and Gas in the Small Magellanic Cloud
Published online by Cambridge University Press: 25 May 2016
Extract
Here we present four IRAS high resolution images of the Small Magellanic Cloud, as reconstructed by the HIRAS program using the Pyramid Maximum Entropy method (Bontekoe et al. 1994). (HIRAS is not to be confused with HiRes (Aumann et al. 1990).) The images show much more detail than in Schwering & Israel (1990). Dust temperatures range from 25–41 K (Stanimirović et al. in prep).
- Type
- Part 2. Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 122 - 123
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
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