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arXiv · 1211.5206

Competitive accretion in the protocluster G10.6-0.4?

Tie Liu·Yuefang Wu·Jingwen Wu·Sheng-Li Qin·Huawei Zhang
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Abstract

We present the results of high spatial resolution observations at 1.1 mm waveband, with the Submillimetre Array (SMA), towards the protocluster G10.6-0.4. The 1.1 mm continuum emission reveals seven dense cores, towards which infall motions are all detected with the red-shifted absorption dips in HCN (3--2) line. This is the first time that infall is seen towards multiple sources in a protocluster. We also identified four infrared point sources in this region, which are most likely Class 0/I protostars. Two jet-like structures are also identified from Spitzer/IRAC image. The dense core located in the centre has much larger mass than the off-centre cores. The clump is in overall collapse and the infall motion is supersonic. The standard deviation of core velocities and the velocity differences between the cores and the cloud/clump are all larger than the thermal velocity dispersion. The picture of G10.6-0.4 seems to favor the "competitive accretion" model but needs to be tested by further observations.

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Tie Liu, Yuefang Wu, Jingwen Wu, Sheng-Li Qin, Huawei Zhang. 2012-11-22. Competitive accretion in the protocluster G10.6-0.4?. https://doi.org/10.1093/mnras%2Fstt1650

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