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| Query : 2011NewA...16..323A |
2011NewA...16..323A - New Astronomy, 16, 323-327 (2011)
On the propensity of the formation of massive clumps via fragmentation of driven shells.
ANATHPINDIKA S.
Journal keyword(s):
Simbad objects: 4
| Number of rows : 4 |
| 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 | RCW 34 | HII | 08 56 28.1 | -43 05 58 | 10.5 | 11.21 | ~ | 99 | 0 | |||
| 2 | GRS G308.60 +00.60 | HII | 13 39.9 | -61 45 | ~ | 108 | 0 | |||||
| 3 | SH 2-3 | HII | 17 12.4 | -38 28 | ~ | 234 | 1 | |||||
| 4 | [L89b] 28.823-00.226 | bub | 18 44 44.3 | -03 45 34 | ~ | 80 | 0 |
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