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| Query : 1994ApJ...423..326B |
1994ApJ...423..326B - Astrophys. J., 423, 326-333 (1994/March-1)
Spectral imaging of the Orion bar at 3.3, 8.4 and 11.3 microns : comparison with a fluorescent polycyclic aromatic hydrocarbon model.
BREGMAN J., LARSON K., RANK D. and TEMI P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): ISM: Dust, Extinction - Infrared: ISM: Continuum - ISM: Individual Name: Orion Nebula - ISM: Molecules
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 | M 42 | HII | 05 35 16.8 | -05 23 15 | ~ | 4411 | 0 | |||||
| 2 | NAME Orion Bright Bar | reg | 05 35 22.30 | -05 24 33.0 | ~ | 1004 | 0 |
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