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A New CO Outflow Source near NGC 2071
Published online by Cambridge University Press: 04 August 2017
Extract
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
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- Copyright © Reidel 1987