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| Query : 1983MNRAS.205..389W |
1983MNRAS.205..389W - Mon. Not. R. Astron. Soc., 205, 389-393 (1983)
Is emission line strength a predictor of youth for Orion population stars ?
WEAVER W.B.
Journal keyword(s):
Simbad objects: 6
| Number of rows : 6 |
| 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 Tau-Aur Complex | SFR | 04 30 | +25.0 | ~ | 1453 | 0 | |||||
| 2 | M 42 | HII | 05 35 16.8 | -05 23 15 | ~ | 4411 | 0 | |||||
| 3 | NAME Ori A | MoC | 05 38 | -07.1 | ~ | 3187 | 0 | |||||
| 4 | NGC 2264 | OpC | 06 40 53.7 | +09 52 32 | ~ | 1876 | 0 | |||||
| 5 | IC 5070 | HII | 20 51.0 | +44 22 | ~ | 218 | 1 | |||||
| 6 | NGC 7000 | Cl* | 20 58 47 | +44 19.8 | ~ | 427 | 0 |
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