Stellar Relics of the hierarchical assembly of the Galaxy

This PhD Thesis is part of a long-term wide research project, carried out by the "Osservatorio Astronomico di Bologna (INAF-OABO)", that has as primary goal the comprehension and reconstruction of formation mechanism of galaxies and their evolution history. There is now substantial evidence, both from theoretical and observational point of view, in favor of the hypothesis that the halo of our Galaxy has been at least partially, built up by the progressive accretion of small fragments, similar in nature to the present day dwarf galaxies of the Local Group. In this context, the photometric and spectroscopic study of systems which populate the halo of our Galaxy (i.e. dwarf spheroidal galaxy, tidal streams, massive globular cluster, etc) permits to discover, not only the origin and behaviour of these systems, but also the structure of our Galactic halo, combined with its formation history. In fact, the study of the population of these objects and also of their chemical compositions, age, metallicities and velocity dispersion, permit us not only an improvement in the understanding of the mechanisms that govern the Galactic formation, but also a valid indirect test for cosmological model itself. Specifically, in this Thesis we provided a complete characterization of the tidal Stream of the Sagittarius dwarf spheroidal galaxy, that is the most striking example of the process of tidal disruption and accretion of a dwarf satellite in to our Galaxy. Using Red Clump stars, extracted from the catalogue of the Sloan Digital Sky Survey (SDSS) we obtained an estimate of the distance, the depth along the line of sight and of the number density for each detected portion of the Stream (and more in general for each detected structure along our line of sight). Moreover comparing the relative number (i.e. the ratio) of Blue Horizontal Branch stars and Red Clump stars (the two features are tracers of different age/different metallicity populations) in the main body of the galaxy and in the Stream, in order to verify the presence of an age-metallicity gradient along the Stream. We also report the detection of a population of Red Clump stars probably associated with the recently discovered Bootes III stellar system. Finally, we also present the results of a survey of radial velocities over a wide region, extending from r ~ 10' out to r ~ 80' within the massive star cluster Omega Centauri. The survey was performed with FLAMES@VLT, to study the velocity dispersion profile in the outer regions of this stellar system. All the results presented in this Thesis, have already been published in refeered journals.

Anomalie cerebellari fetali: confronto tra ecografia e risonanza magnetica prenatale e follow up a distanza

Cerebellar malformation are increasingly diagnosed in utero. To assess the effectiveness of ultrasound and fetal magnetic resonance in the antenatal prediction of long term neurodevelopmental delay. STUDY DESIGN: We collected 105 cases of cerebellum malformation in the period 2000-2010 in Bologna and Bari University. Classification included cystic anomalies of posterior fossa and cerebellar hypoplasia. RESULTS: The greater group included Blake’s pouch cysts and mega cisterna magna cases (58/105). These cases seemed to have a good prognosis with a good outcome both in association with other anomalies and isolated. In cases of Dandy Walker malformation, vermis hypoplasia and cerebellum hypoplasia there were few survivors, so it was so difficult to outline some conclusion for child outcome. Despite great neuroimaging advances, in our study, ultrasound and MR reached a similar sensitivity (62-63%) for the diagnosis of posterior fossa anomalies, but the number of MR was lower compared with ultrasonography. CONCLUSION: Ultrasonography remains the screening method of choice for evaluation of cerebellum anatomy but probably MR imaging can improve some details expecially in the third trimester. Despite the data on Dandy Walker, vermis hypoplasia and cerebellum hypoplasia were conflicting and uncertain, for Blake and mega cisterna magna we can considered a rather good outcome.

Il ruolo dell’ecografia prenatale nella diagnosi precoce delle anomalie fetali della fossa cranica posteriore

Obiettivo: Valutare il ruolo brainstem-vermis angle (BV angle) a 16-18 settimane per la diagnosi precoce delle anomalie cistiche della fossa cranica posteriore. Metodi: Uno studio prospettico, multicentrico, osservazionale. Volumi ecografici tridimensionali della testa fetale sono stati acquisiti in feti a 16-18 settimane. Tre operatori di simile esperienza hanno misurato il BV angle nel piano sagittale come precedentemente descritto1,2 e hanno annotato se il quarto ventricolo era aperto sul piano assiale. Un follow-up dettagliato è stato ottenuto in tutti i casi. Risultati: Tra novembre 2009 e marzo 2011, 150 volumi sono stati acquisiti ad un’epoca gestazionale media di 16 settimane. A causa di una scarsa qualità delle immaginai, 49 volumi sono stati esclusi, con una popolazione finale di 101 casi. Di questi, 6 hanno ricevuto successivamente una diagnosi di malformazione di Dandy-Walker (DWM) e 2 di cisti della tasca di Blake (BPC), gli altri erano normali. In tutti i feti con anomalie cistiche della fossa cranica posteriore, il BV angle è risultato significativamente più ampio rispetto ai controlli (57.3+23.0° vs 9.4+7.7°, U-Mann Whitney test p<0.000005). Nel 90.3% dei feti normali, il BV angle era <20° e il quarto ventricolo era chiuso sul piano assiale. In 9 feti normali e nei casi con BPC, l’angolo era >20° ma <45° (25.8+5.6°) e il quarto ventricolo era aperto posteriormente sul piano assiale, ma solo utilizzando una scansione non convenzionale. In tutti i feti con DWM, il BV angle era >45° (67.9+13.9°) e il quarto ventricolo era aperto anche sul piano assiale standard. Conclusioni: Fino ad ora la diagnosi di anomalie cistiche della fossa cranica posteriore è stata consideratea difficile o impossibile prima di 20 settimane, a causa del presunto sviluppo tardivo del verme cerebellare. La nostra esperienza suggerisce che la misurazione del BV angle consente un’identificazione precisa di queste condizioni già a 16 settimane.