The pincushion cloud - The bipolar flows in L988

Details The pincushion cloud - The bipolar flows in L988 The pincushion cloud - The bipolar flows in L988

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...164l..19c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 164, no. 2, Aug. 1986, p. L19-L21.

Astronomy and Astrophysics

Astronomy

12

Infrared Astronomy, Molecular Flow, Protostars, Star Formation, Astronomical Models, Carbon Monoxide, Infrared Astronomy Satellite, Infrared Stars, Rotating Plasmas

Scientific paper

Four spatially resolved high velocity molecular flows have been detected in the dark cloud L988, three of which are clearly bipolar. The central infrared sources of the flows are visible. The three flows reported here are not parallel with each other, suggesting that the mechanism collimating the flows on the parsec scale may not necessarily be global rotation or magnetic field. Rather the projected blueshifted lobes all seem to point away from each other.

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