The Collimated Bipolar Outflow of OH231.8+4.2

Details The Collimated Bipolar Outflow of OH231.8+4.2 The Collimated Bipolar Outflow of OH231.8+4.2

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.6302f&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #63.02; Bulletin of the American Astronomical Society, Vol. 28, p.1352

Astronomy and Astrophysics

Astronomy

Scientific paper

We present high resolution (5") CO J=1-0 line observations of the bipolar nebula OH231.8+4.2 taken with the BIMA millimeter array. The integrated CO intensity map reveals a highly collimated molecular jet along the polar axis, aligned with the red and blue-shifted bipolar lobes. A constant velocity gradient along the entire length of the bipolar axis is also seen. The de-projected CO outflow velocity exceeds 120 km/s which suggests a dynamical age of 900 years.

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