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| Query : 1999ApJ...515..249O |
1999ApJ...515..249O - Astrophys. J., 515, 249-255 (1999/April-2)
A high-velocity molecular cloud near the center of the Galaxy.
OKA T., WHITE G.J., HASEGAWA T., SATO F., TSUBOI M. and MIYAZAKI A.
Abstract (from CDS):
New observations with the James Clerk Maxwell Telescope 15 m and the NRO 45 m telescopes show that CO 0.02-0.02 is very bright in the CO (J=3-2) and in the HCN and HCO+ (J=1-0) lines. It appears that the environment may have an unusually high density and temperature, which may be related to the very broad CO line width.
We propose that CO 0.02-0.02 may have been accelerated, heated, and compressed in a series of supernovae shocks that have occurred within the last (3-5)x104 yr.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: Center - ISM: Clouds - ISM: Molecules
Simbad objects: 7
| Number of rows : 7 |
| 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 NGC 6334-I | Cl* | 17 20 53.35 | -35 47 01.5 | ~ | 373 | 0 | |||||
| 2 | Bania Clump 1 | MoC | 17 30.7 | -33 18 | ~ | 19 | 1 | |||||
| 3 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 16269 | 0 | |||||
| 4 | NAME Sgr A* | X | 17 45 40.03599 | -29 00 28.1699 | ~ | 4970 | 3 | |||||
| 5 | CO 000.02-00.02 | MoC | 17 45.7 | -28 56 | ~ | 34 | 0 | |||||
| 6 | CO 000.13-00.13 | MoC | 17 46.4 | -28 54 | ~ | 24 | 0 | |||||
| 7 | Bania Clump 2 | MoC | 17 51 42.6 | -26 17 18 | ~ | 41 | 1 |
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