The chemical composition of interstellar molecular clouds.
Relative abundances for molecules observed by radio astronomical techniques have been determined for several interstellar regions with differing physical properties.
Irvine
W M
WM
Astronomy Program, University of Massachusetts, Amherst 01003, USA.
Hjalmarson
A
A
D001256:Astronomy / Q000379:methods*; D002248:Carbon Monoxide / Q000032:analysis; D019418:Evolution, Chemical; D005118:Extraterrestrial Environment; D005740:Gases / Q000032:analysis*; D006859:Hydrogen / Q000032:analysis; D006856:Hydrogen Cyanide / Q000032:analysis; D009570:Nitriles / Q000032:analysis; D013057:Spectrum Analysis
D005740:Gases; D009570:Nitriles; D006856:Hydrogen Cyanide; D002248:Carbon Monoxide; D006859:Hydrogen