Molecular outflows in the L1641 region of Orion

Details Molecular outflows in the L1641 region of Orion Molecular outflows in the L1641 region of Orion

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...372..505m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 372, May 10, 1991, p. 505-517.

Astronomy and Astrophysics

Astronomy

28

Infrared Sources (Astronomy), Interstellar Matter, Molecular Flow, Nebulae, Carbon Compounds, Color-Color Diagram, Emission Spectra, Infrared Astronomy Satellite, Spectral Emission

Scientific paper

Searches for high-velocity C-12O emission from possible molecular-outflow candidates, and CS emission from dense cores in the vicinity of each IRAS source, were conducted during a mm-wave survey of a flux-limited sample of IRAS sources within a 4 sq deg region of the L1641 portion of the Orion A molecular cloud. The C-12O line emission width is noted to be correlated with the strength of the integrated CS emission. Attention was given to the IR properties of the embedded sources; the molecular outflow candidate sources have generally redder 12-25 micron colors and bluer 60-100 micron colors than the nonmolecular outflow candidates.

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