The Dusty Envelope of L 723 at Sub-mm Wavelengths

Details The Dusty Envelope of L 723 at Sub-mm Wavelengths The Dusty Envelope of L 723 at Sub-mm Wavelengths

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..135e&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

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4

Ism: Clouds, Ism: Dust, Ism: Individual: L723, Ism: Structure, Stars: Formation

Scientific paper

L 723 has an associated CO outflow with a quadrupolar morphology (Goldsmith et al. 1984; Lee et al. 2002). The larger pair of lobes is aligned in an east-west direction, while the other pair is roughly in a north-south direction. The powering source of the large east-west outflow is IRAS 19156+1906, associated with the thermal radio jet VLA 2 (Anglada et al. 1991; Anglada, Rodríguez, & Torrelles 1997).

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