Identifying and characterising young, nearby, low-mass members of stellar moving groups
Since the early 1990s, several groups of comoving, coeval stars younger than 100Myr and within 100 pc have been revealed. Studying and identifying members in these ‘Nearby Young Moving Groups’ (MGs) is vital because they provide: well characterised samples to test pre-main sequence evolution; ideal...
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Keele University
2015
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.695580 |