Pulsating variable stars as tracers of galactic structure and interaction mechanisms


Autoria(s): Moretti, Maria Ida
Contribuinte(s)

Marano, Bruno

Data(s)

20/04/2012

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