We have spectrophotometrically observed twenty M-class asteroids in the 1.2-to 3.5-µm region, sixteen of them for the first time. When we combined these with earlier surveys by Rivkin et al. (1995) and Jones et al. (1990) for a total of 27 asteroids, we find that over 35% of them have absorption fea
Observations of asteroids in the 3- to 4-μm region
✍ Scribed by N. Eaton; S.F. Green; R.S. McCheyne; A.J. Meadows; G.J. Veeder
- Publisher
- Elsevier Science
- Year
- 1983
- Tongue
- English
- Weight
- 355 KB
- Volume
- 55
- Category
- Article
- ISSN
- 0019-1035
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