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| Query : 1998ApJ...501..207T |
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
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | TMC-1 | MoC | 04 41 45.9 | +25 41 27 | ~ | 1872 | 0 | |||||
| 2 | LDN 183 | MoC | 15 54 12.2 | -02 49 42 | ~ | 799 | 1 |
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