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1998ApJ...501..207T - Astrophys. J., 501, 207-220 (1998/July-1)
The sensitivity of gas-phase chemical models of interstellar clouds to C and O elemental abundances and to a new formation mechanism for ammonia.
TERZIEVA R. and HERBST E.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): ISM: Abundances - ISM: Clouds - ISM: Molecules - Molecular Processes
Simbad objects: 2
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