Published October 1982 | Version v1
Journal article

Westerbork observations of 6-cm H2CO in W3

  • 1. Rijksuniversiteit Groningen (Netherlands). Kapteyn Sterrewacht
  • 2. Illinois Univ., Urbana (USA). Dept. of Astronomy
  • 3. Dwineloo Observatory (Netherlands)

Description

The distribution of the 4.8-GHz formaldehyde absorption against the continuum sources in the W3 core has been mapped with an angular resolution of 8.2 x 9.3 arcsec2 and a velocity resolution of 1.22 km s-1. Opacity variations on a linear scale size of 0.2 pc are seen against the continuum source W3A. The opacity enhancements are interpreted as being caused by clumping in the molecular material overlying the continuum source. There is a strong correlation between the optical depth of H2CO and that of the silicate absorption at 9.7 μm. Evidence for an interaction between the ionized gas and the surrounding molecular cloud has been found. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
201
Journal Issue
1
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
317-330
ISSN
0035-8711