CN zeeman observations of molecular cloud cores

Richard M. Crutcher, Thomas H. Troland, Bernard Lazareff, Ilya Kazès

Research output: Contribution to journalArticlepeer-review

Abstract

We present results from the first attempt to measure strengths of magnetic fields in dense molecular cloud cores by observations of the Zeeman effect in the 3 mm lines of CN. The observations were made with the 30 m IRAM radio telescope with a new polarimeter constructed for this experiment. The two molecular cores which were observed are located about 3′ north of Orion-KL (OMC-N4) and about 1′ east of IRS 4 in S106 (S106-CN). From CN data for OMC-N4 and S106-CN, respectively, we estimate cloud radii of 0.03 and 0.05 pc, masses of 10 and 22 M, and H2 densities of 1.6 × 106 cm-3. Our CN Zeeman results for the line-of-sight magnetic fields are Blos(OMC-N4) = +79 ± 99 μG and Blos(S106-CN) = -57 ±199 μG. Hence, we did not detect magnetic fields. Our upper limits for Blos are significantly less than field strengths expected for assumption of internal motions at the Alfvén speed, of a critical mass to magnetic flux ratio, or of virial equilibrium, but the very small sample of clouds and the uncertainties in the |B|Alfvén' |B|critical' and |B|virial estimates preclude definite conclusions.

Original languageEnglish (US)
Pages (from-to)217-224
Number of pages8
JournalAstrophysical Journal
Volume456
Issue number1 PART I
DOIs
StatePublished - 1996

Keywords

  • ISM: Clouds
  • ISM: Magnetic fields
  • ISM: Molecules
  • Polarization

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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