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A New CO Outflow Source near NGC 2071

Published online by Cambridge University Press:  04 August 2017

T. Iwata  and
Y. Fukui
T. Iwata
Affiliation:
Nagoya University, Japan
Y. Fukui
Affiliation:
Nagoya University, Japan

Extract

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The region of NGC 2071 and NGC 2068 is one of the active sites of star formation in Orion. An extended CO cloud in this region has been studied previously (e.g., White et al. 1981). Here, we report new J = 1-0 CO, 13 CO, and C18 O observations of this region with a 2.7′ beam. Up to the present, we have obtained 400, 800, and 100 spectra for CO, 13 CO, and C18 O lines, respectively. The data cover an area of ∼ 1°x2°.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 357
Copyright
Copyright © Reidel 1987