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| Query : 1994Ap&SS.217..195L |
1994Ap&SS.217..195L - Astrophys. Space Sci., 217, 195-197 (1994)
Are molecular clouds formed by impact of high-velocity clouds ?
LEPINE J.R.D. and DUVERT G.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| 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 Taurus Complex | SFR | 04 41.0 | +25 52 | ~ | 4971 | 0 | |||||
| 2 | * lam Ori | ** | 05 35 08.27761 | +09 56 02.9611 | 2.45 | 3.48 | 3.66 | 3.72 | 3.89 | O8IIIf+B0.5V | 327 | 0 |
| 3 | NAME Ori Complex | Cld | 05 35.3 | -05 23 | ~ | 481 | 0 | |||||
| 4 | NAME Chamaeleon Region | SFR | 11 55 | -78.0 | ~ | 887 | 0 | |||||
| 5 | NAME Ophiuchus Molecular Cloud | SFR | 16 28 06 | -24 32.5 | ~ | 3969 | 1 |
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