The link between solenoidal turbulence and slow star formation in G0.253+0.016

The link between solenoidal turbulence and slow star formation in G0.253+0.016

Star formation in the Galactic disc is primarily controlled by gravity, turbulence, and magnetic fields. It is not clear that this also applies to star formation near the Galactic Centre. Here we determine the turbulence and star formation in the CMZ cloud G0.253+0.016. Using maps of 3 mm dust emiss...

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Bibliographic Details
Main Authors: Federrath, C., Rathborne, J., Longmore, S., Kruijssen, J., Bally, J., Contreras, Y., Crocker, R., Garay, G., Jackson, J., Testi, L., Walsh, Andrew
Format: Conference Paper
Published: 2016
Online Access:http://hdl.handle.net/20.500.11937/50759

Internet

http://hdl.handle.net/20.500.11937/50759

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