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Molecular outflows associated with GL 2591 and W28 A2 were observed in the492 GHz [CI] line. Upper limits are set on the [CI] emission in the extremelyhigh velocity line wings. These limits are discussed in terms of wind-drivenand jet-driven models of molecular outflows.Comment: 9 pages (7 texts + 2 figures) Prepared with the AAS LaTeX macro v3.

Observation of (C I) toward the GL 2591 and W28 A2 molecular outflows