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Pulsating stars in the VMC survey

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 نشر من قبل Maria-Rosa Cioni Dr.
 تاريخ النشر 2017
  مجال البحث فيزياء
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The VISTA survey of the Magellanic Clouds system (VMC) began observations in 2009 and since then, it has collected multi-epoch data at Ks and in addition multi-band data in Y and J for a wide range of stellar populations across the Magellanic system. Among them are pulsating variable stars: Cepheids, RR Lyrae, and asymptotic giant branch stars that represent useful tracers of the host system geometry.



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