The magnetic field of the NGC 2024 molecular cloud - Detection of OH line Zeeman splitting

Details The magnetic field of the NGC 2024 molecular cloud - Detection of OH line Zeeman splitting The magnetic field of the NGC 2024 molecular cloud - Detection of OH line Zeeman splitting

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...125l..23c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 125, no. 2, Sept. 1983, p. L23-L26. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

46

Hydroxyl Emission, Interstellar Magnetic Fields, Line Spectra, Molecular Clouds, Zeeman Effect, Interstellar Matter, Magnetic Flux, Radio Spectra, Splitting

Scientific paper

Zeeman splitting of the main lines of OH in absorption has been detected
for the first time. The derived magnetic field for a clump in the NGC
2024 molecular cloud is -38 plus or minus 1 microgauss.

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