Line polarization of molecular lines at radio frequencies: The case of DR 21(OH)

P. C. Cortes, R. M. Crutcher, W. D. Watson

Research output: Contribution to journalArticle

Abstract

We present polarization observations in DR 21(OH) from thermal dust emission at 3 mm and from CO J = 1 → 0 line emission. The observations were obtained using the Berkeley-Illinois-Maryland Association (BIMA) array. Lai et al. observed this region at 1.3 mm for the polarized continuum emission and also measured the CO J = 2 → 1 polarization. Our continuum polarization results are consistent with those of Lai et al. However, the direction of the linear polarization for the J = 1 → 0 is perpendicular to that of the CO J = 2 → 1 polarization. This unexpected result was explored by obtaining numerical solutions to the multilevel radiative transfer equations for a gas with anisotropic optical depths. We find that in addition to the anisotropic optical depths, anisotropic excitation due to a source of radiation that is external to the CO is needed to understand the orthogonality in the directions of polarization. The continuum emission by dust grains at the core of DR 21 (OH) is sufficient to provide this external radiation. The CO polarization must arise in relatively low density (nH2 ∼ 100 cm-3) envelope gas. We infer B ∼ 10 μG in this gas, which implies that the envelope is subcritical.

Original languageEnglish (US)
Pages (from-to)780-788
Number of pages9
JournalAstrophysical Journal
Volume628
Issue number2 I
DOIs
StatePublished - Aug 1 2005

Keywords

  • ISM: magnetic fields
  • ISM: molecules
  • Polarization
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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