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Pulsating variable stars as tracers of galactic structure and interaction mechanisms

My PhD project has been focused on the study of the pulsating variable stars
in two ultra-faint dwarf spheroidal satellites of the Milky Way, namely, Leo IV and
Hercules; and in two fields of the Large Magellanic Cloud (namely, the Gaia South
Ecliptic Pole calibration field, and the 30 Doradus region) that were repeatedly
observed in the KS band by the VISTA Magellanic Cloud (VMC, PI M.R. Cioni)
survey of the Magellanic System.

Identiferoai:union.ndltd.org:unibo.it/oai:amsdottorato.cib.unibo.it:4770
Date20 April 2012
CreatorsMoretti, Maria Ida <1982>
ContributorsMarano, Bruno
PublisherAlma Mater Studiorum - Università di Bologna
Source SetsUniversità di Bologna
LanguageEnglish
Detected LanguageEnglish
TypeDoctoral Thesis, PeerReviewed
Formatapplication/pdf
Rightsinfo:eu-repo/semantics/openAccess

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