Molecular emission in regions of star formation
Recent observations show that young stars being formed eject matter at several tens of kilometers per second, in the form of jets and outflows that impact the matter whose collapse is at the origin of the formation of the star. The supersonic impact between this jet and the parent interstellar cloud...
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Durham University
2008
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.492852 |