Magnetic fields in molecular clouds - OH Zeeman observations

Details Magnetic fields in molecular clouds - OH Zeeman observations Magnetic fields in molecular clouds - OH Zeeman observations

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249..134c&link_type=abstract

Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 134-137.

Astronomy and Astrophysics

Astrophysics

19

Absorption Spectra, Hydroxyl Radicals, Interstellar Magnetic Fields, Molecular Clouds, Zeeman Effect, Field Strength, H Lines, Power Spectra

Scientific paper

OH Zeeman observations of the absorption lines produced in interstellar dust clouds toward 3C 133, 3C 123 and W51 lead to conservative, 3 sigma upper limits to the magnetic field at each position of 15, 25 and 30 microgauss, respectively. The line spectrum and the polarization-switched Zeeman spectrum were computed for each source using only normalized power spectra derived from the autocorrelation receiver.

Affiliated with

Also associated with

No associations

Rating

Magnetic fields in molecular clouds - OH Zeeman observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Magnetic fields in molecular clouds - OH Zeeman observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic fields in molecular clouds - OH Zeeman observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1468523