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| Query : 1996ApJ...463L.113H |
1996ApJ...463L.113H - Astrophys. J., 463, L113-L116 (1996/May-3)
Why HOC+ is detectable in interstellar clouds: the rate of the reaction between HOC+ and H2.
HERBST E. and WOON D.E.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): ISM: Abundances - ISM: Clouds - ISM: Molecules - Molecular Processes
Errata: 1996ApJ...471L..73H
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 | NAME Orion-KL | SFR | 05 35 14.16 | -05 22 21.5 | ~ | 2421 | 1 | |||||
| 2 | NAME Sgr B2 (OH) | MoC | 17 47 20.8 | -28 23 32 | ~ | 91 | 0 |
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