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| Query : 2004ApJ...616L.111H |
2004ApJ...616L.111H - Astrophys. J., 616, L111-L114 (2004/December-1)
Evaluating the magnetic field strength in molecular clouds.
HOUDE M.
Abstract (from CDS):
We discuss an extension to the Chandrasekhar-Fermi method for the evaluation of the mean magnetic field strength in molecular clouds to cases where the spatial orientation of the field is known. We apply the results to M17, using previously published data.
Abstract Copyright: ∼
Journal keyword(s): ISM: Clouds - ISM: Individual: Messier Number: M17 - ISM: Magnetic Fields - Polarization
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 - 2024 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | M 42 | HII | 05 35 17 | -05 23.4 | ~ | 4079 | 0 | |||||
| 2 | NAME Ori A | MoC | 05 38 | -07.1 | ~ | 3014 | 0 | |||||
| 3 | NGC 6618 | OpC | 18 20 47 | -16 10.3 | ~ | 1615 | 0 | |||||
| 4 | DR 21 (OH) | cor | 20 39 01.01 | +42 22 50.2 | ~ | 410 | 0 |
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