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The Extinction Efficiency of Dust Grains at 1 Mm
Published online by Cambridge University Press: 14 August 2015
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We have determined the extinction efficiency factor Q for the objects in the Table by means of maps, scans, or photometry at 1 mm using a composite bolometer at the prime focus of the ESO 3.6m telescope (Arnold et al., 1978; Arnold, 1979). The beam is 2′ in diameter.
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- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 133 - 134
- Copyright
- Copyright © Reidel 1980
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