Zeeman splitting in interstellar molecules

Details Zeeman splitting in interstellar molecules Zeeman splitting in interstellar molecules

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224..206b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 206-208.

Astronomy and Astrophysics

Astrophysics

5

Diatomic Molecules, Interstellar Matter, Magnetic Fields, Zeeman Effect, Cyanogen, Millimeter Waves, Radio Telescopes, Sulfur Oxides

Scientific paper

The Zeeman splitting due to a longitudinal magnetic field on some transitions of diatomic molecules observed in the interstellar clouds are calculated. Only CN and SO exhibit effects comparable to that of OH. Their observability in the mm range is discussed. In the same wavelength range, O2 would exhibit Zeeman effects even larger than that of OH, but must be observed from space radiotelescopes.

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