Gas infall in the massive star formation core G192.16-3.84
arXiv:1810.01597 · doi:10.1088/1674-4527/19/3/40
Abstract
Previous observations have revealed an accretion disk and outflow motion in high-mass star-forming region G192.16-3.84. While collapse have not been reported before. We present here molecular line and continuum observations toward massive core G192.16-3.84 with the Submillimeter Array. CO(2-1) and HCO(3-2) lines show pronounced blue profiles, indicating gas infalling in this region. This is the first time that the infall motion has been reported in G192.16-3.84 core. Two-layer model fitting gave infall velocities of 2.00.2 and 2.80.1 km s. Assuming that the cloud core follows a power-law density profile (), the corresponding mass infall rates are (4.71.7) and (6.62.1) M$_{\sun}$ yr for CO(2-1) and HCO(3-2), respectively. The derived infall rates are in agreement with the turbulent core model and those in other high-mass star-forming regions, suggesting that high accretion rate is a general requirement to form a massive star.
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