The Orion-IRc2 Outflow Observed in CO J=4-3

Details The Orion-IRc2 Outflow Observed in CO J=4-3 The Orion-IRc2 Outflow Observed in CO J=4-3

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..143s&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 143-149

Astronomy and Astrophysics

Astrophysics

Scientific paper

A CO J=4-3 map of the Orion-IRc2 region (size 80″, beam 15″) is presented. The outflow has a bipolar structure observed nearly pole-on. We interpret our observations in terms of an hierarchy of “tubes” where the fastest gas proceeds through the narrowest, innermost cone. The gas has an inhomogeneous temperature distribution and must be highly clumped. Most of the properties derived comply with the picture developed for the few known extreme high velocity outflows; however, this outflow contains exceptionally dense gas ( > 106 cm-3).

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