Abstract Relative abundances for molecules observed by radio astronomical techniques have been determined for several interstellar regions with differing physical properties.
The chemical composition of interstellar molecular clouds
Origins of life ; 14 , 1-4
1984
Article (Journal)
English
BKL: | 44.71 Verkehrsmedizin | |
Local classification TIB: | 535/3908/4290 |
Fragmentation of magnetised filamentary interstellar clouds
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