Pulsating variable stars as tracers of galactic structure and interaction mechanisms
Contribuinte(s) |
Marano, Bruno |
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Data(s) |
20/04/2012
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Resumo |
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. |
Formato |
application/pdf |
Identificador |
http://amsdottorato.unibo.it/4770/1/Moretti_MariaIda_tesi.pdf urn:nbn:it:unibo-4247 Moretti, Maria Ida (2012) Pulsating variable stars as tracers of galactic structure and interaction mechanisms, [Dissertation thesis], Alma Mater Studiorum Università di Bologna. Dottorato di ricerca in Astronomia <http://amsdottorato.unibo.it/view/dottorati/DOT203/>, 24 Ciclo. DOI 10.6092/unibo/amsdottorato/4770. |
Idioma(s) |
en |
Publicador |
Alma Mater Studiorum - Università di Bologna |
Relação |
http://amsdottorato.unibo.it/4770/ |
Direitos |
info:eu-repo/semantics/openAccess |
Palavras-Chave | #FIS/05 Astronomia e astrofisica |
Tipo |
Tesi di dottorato NonPeerReviewed |