Infrared and optical studies of cool low-mass dwarfs
Infrared and optical studies of cool low-mass dwarfs are made in order to determine their properties. The goal of distinguishing low-mass stars from brown dwarfs is engaged by studies on a number of different fronts. (1) The first infrared spectral sequence of cool dwarfs from GL411 (M2V) to GD165B...
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University of Edinburgh
1995
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.653133 |