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Keywords

ISM: clouds
ISM: dust
ISM: individual: L723
ISM: structure
Stars: formation

How to Cite

The Dusty Envelope of L 723 at Sub-mm Wavelengths. (2003). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 15(1), 135-135. https://astronomia.unam.mx/journals/rmxac/article/view/2003rmxac..15..135e
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Abstract

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).