作者: Kazuya Saigo , Patricio Sanhueza , Aya E. Higuchi , Tetsuo Hasegawa , James O. Chibueze
DOI: 10.1088/0004-637X/815/2/106
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摘要: We present the results of SiO (2-1) and SO2 (12-13) line observations Sgr B2(N) made with Atacama Large Millimeter/submillimeter Array (ALMA) at an angular resolution ~2arcsec. Our analysis emission reveals a bipolar molecular outflow in east-west direction whose driving source is located K2. In addition, core shows north-south velocity gradient most probably indicating hot gas rotating around Fractional abundances (X(SO2) X(SiO), respectively) outflowing are derived from comparisons C18O emission. Assuming excitation temperature 100+-50 K, we calculate X(SO2) = 2.3X10^-8 X(SiO) 1.2X10^-9. The SgrB2(N) K2 characterized as young (5X10^3yr) massive (~2000Msun), but moderately collimated (~60deg) outflow. also report possible detection (v=2, J=2-1) maser position If confirmed, it would make 4th star forming region associated masers.