The magnetic field of the NGC 2024 molecular cloud

R. M. Crutcher, D. A. Roberts, T. H. Troland, W. M. Goss

Research output: Contribution to journalArticlepeer-review

Abstract

We have carried out Very Large Array (VLA)1 Zeeman observations of absorption lines of H I and OH toward the molecular cloud associated with the NGC 2024 (Orion B) H II region. The synthesized beam diameters are 68″ × 52″, p.a. = 38°, and 81″ × 65″, p.a. = -6°, for OH and H I, respectively. The absorption lines could be mapped over the NGC 2024 continuum source, which has an extent (at the 1 Jy beam-1 level) of Δα ≈ 7′ by Δδ ≈ 5′. The maps of the magnetic field, together with comparisons with additional data from the published literature, lead to the following conclusions: (1) The magnetic field comes from a line subcomponent at vLSR ≈ 10.2 km s-1, which corresponds in velocity and in spatial morphology with the northern dense molecular ridge in NGC 2024. (2) Blos varies from 0 to the northeast of the northern molecular ridge to almost 100 μG to the southwest. The variation in Blos may be due to the field being mainly in the plane of the sky to the northeast but having a significant line-of-sight component to the southwest. (3) Velocities in the cloud are supersonic but approximately equal to the Alfvén velocity, which is consistent with motions being dominated by magnetohydrodynamical waves rather than thermal motion or hydrodynamical turbulence. (4) The mass-to-magnetic flux ratio is super-critical, which suggests that the static magnetic field does not support the cloud against collapse. Simple virial estimates of the relative importance of gravitational, kinetic, and magnetic energies show that the ratio of kinetic/gravitational energy is about 0.5, while the magnetic/gravitational energy ratio is less than 0.1. At face value, these results imply that the cloud is supported mainly by nonthermal motions rather than by the static magnetic field. However, since we only measure directly the line-of-sight component of B, this result is not conclusive.

Original languageEnglish (US)
Pages (from-to)275-285
Number of pages11
JournalAstrophysical Journal
Volume515
Issue number1 PART 1
DOIs
StatePublished - Apr 10 1999

Keywords

  • ISM: clouds
  • ISM: kinematics and dynamics
  • ISM: magnetic fields
  • ISM: molecules
  • Ism: individual (NGC 2024)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'The magnetic field of the NGC 2024 molecular cloud'. Together they form a unique fingerprint.

Cite this