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- W2012120163 abstract "We present the results of a high resolution study with the Submillimeter Array towards the massive star forming complex G9.62+0.19. Three sub-mm cores are detected in this region. The masses are 13, 30 and 165 M$_{sun}$ for the northern, middle and southern dust cores, respectively. Infall motions are found with HCN (4-3) and CS (7-6) lines at the middle core (G9.62+0.19 E). The infall rate is $4.3times10^{-3}~M_{odot}cdot$yr$^{-1}$. In the southern core, a bipolar-outflow with a total mass about 26 M$_{sun}$ and a mass-loss rate of $3.6times10^{-5}~M_{odot}cdot$yr$^{-1}$ is revealed in SO ($8_{7}-7_{7}$) line wing emission. CS (7-6) and HCN (4-3) lines trace higher velocity gas than SO ($8_{7}-7_{7}$). G9.62+0.19 F is confirmed to be the driving source of the outflow. We also analyze the abundances of CS, SO and HCN along the redshifted outflow lobes. The mass-velocity diagrams of the outflow lobes can be well fitted by a single power law. The evolutionary sequence of the cm/mm cores in this region are also analyzed. The results support that UC~H{sc ii} regions have a higher blue excess than their precursors." @default.
- W2012120163 created "2016-06-24" @default.
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- W2012120163 date "2011-03-10" @default.
- W2012120163 modified "2023-09-22" @default.
- W2012120163 title "INFALL AND OUTFLOW MOTIONS IN THE HIGH-MASS STAR-FORMING COMPLEX G9.62+0.19" @default.
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- W2012120163 doi "https://doi.org/10.1088/0004-637x/730/2/102" @default.
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