Hostname: page-component-848d4c4894-xfwgj Total loading time: 0 Render date: 2024-06-16T02:30:16.854Z Has data issue: false hasContentIssue false
  • English
  • Français

Comparison of Submillimeter and CO Brightness in Orion and Mon R2

Published online by Cambridge University Press:  14 August 2015

David Cudaback ,
Lawrence Anderson ,
David Lynch  and
James Smith
David Cudaback
Affiliation:
Radio Astronomy Laboratory, University of California, Berkeley
Lawrence Anderson
Affiliation:
Radio Astronomy Laboratory, University of California, Berkeley
David Lynch
Affiliation:
Department of Physics, California Institute of Technology
James Smith
Affiliation:
Department of Physics, California Institute of Technology

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Emission from interstellar dust in L 1641 and Mon R2 was mapped with three arcminute resolution at 400 microns wavelength from White Mountain, California at 3.9 km elevation. Dust brightness distributions and 13CO antenna temperatures are shown below with equal linear scales, emphasizing that the core of Mon R2 is considerably larger and more massive than the core of the Orion region containing OMC-1 and OMC-2. Dust and 13CO brightness distributions for each object are similar, but some of the differences may be real. The differences become accentuated when mass distributions are compared.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 135 - 136
Copyright
Copyright © Reidel 1980 

References

Kutner, M.L., Evans, N.J. II, and Tucker, K.C.: 1976, Ap.J. 209, 452.CrossRefGoogle Scholar
Loren, R. B.: 1977, Ap.J. 215, 129.CrossRefGoogle Scholar
Righini-Cohen, G., and Simon, M.: 1977, Ap.J. 213, 390.CrossRefGoogle Scholar