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Astron. Astrophys. 327, 689-698 (1997)

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Acknowledgements

We remain grateful to Hans Olofsson for calling our attention, several years ago, on the existence of a velocity gradient in this source. Also we wish to thank to Michel Guélin for fruitful comments on the outflow energy. This work has been partially supported by DGICYT, project number PB 93-0048.

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© European Southern Observatory (ESO) 1997

Online publication: April 6, 1998
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