Twin beams from a young B star?

Details Twin beams from a young B star? Twin beams from a young B star?

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...195..193h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 195, no. 1-2, April 1988, p. 193-197.

Astronomy and Astrophysics

Astrophysics

15

B Stars, H Ii Regions, Late Stars, Molecular Clouds, Star Formation, Stellar Winds, Carbon Monoxide, Hydroxyl Emission, Stellar Luminosity

Scientific paper

G 35.2-0.74N is a young star formation region whose H II emission shows the unusual structure of an optically thick central source with collinear, optically thin lobes on either side. It is suggested that these lobes may be a manifestation of opposing beams of stellar wind and/or ultraviolet radiation which originate in the central source and drive the bipolar molecular outflow observed in this object, providing a valuable clue to the origin of such flows.

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