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Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944
Authors:Jin-Long Xu  Jun-Jie Wang National Astronomical Observatories  Chinese Academy of Sciences  Beijing  China  NAOC-TU Joint Center for Astrophysics  Lhasa
Institution:Jin-Long Xu , Jun-Jie Wang National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China,NAOC-TU Joint Center for Astrophysics,Lhasa 850000
Abstract:The mapping observations of CO J = 2-1, CO J = 3-2, 13 CO J = 2-1 and 13 CO J = 3-2 lines in the direction of IRAS 22506+5944 have been made. The results show that the cores in the J = 2-1 transition lines have a similar morphology to those in the J = 3-2 transition lines. Bipolar molecular outflows are verified. The prior IRAS 22506+5944 observations indicated that two IRAS sources and three H 2 O masers were located close to the peak position of the core. One of the IRAS sources may be the driving source ...
Keywords:ISM  jets and outflows-ISM  kinematics and dynamics-ISM  molecules-stars  formation
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