Structural details of the Orion Nebula: Detection of a network of stringlike ionized features

F. Yusef-Zadeh*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

34 Scopus citations

Abstract

We present high-resolution (1″.8 × 1″.6) radio continuum images of the Orion Nebula at 20 cm based on measurements made with the VLA in a number of its configurations. The overall morphology of ionized gas at 20 cm wavelength shows a number of striking new substructures associated with this geometrically complex H II region. On the largest scale, we find a number of linear features, which are considered as new ionization fronts, and which form a 40° angle with respect to the main ionization front known as the "bar" in M42. These features together with the ridge of emission from the optical bar form a conelike appearance whose 5′-10′ envelope is centered near the Trapezium cluster. On a small scale, we report the detection of a web of stringlike features with typical widths of a few arcseconds (≈ 1016 cm) which are concentrated throughout the Trapezium region. These features reveal morphological evidence for production of shocked ionized gas in starforming regions, perhaps driven by powerful winds from mass-losing stars and/or by the shock fronts produced at the edge of expanding H II regions.

Original languageEnglish (US)
Pages (from-to)L19-L22
JournalAstrophysical Journal
Volume361
Issue number1 PART 2
DOIs
StatePublished - Sep 20 1990

Keywords

  • Nebulae: H II regions
  • Nebulae: structure

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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