Dynamical Evolution of Dense Stellar Systems from Blue Straggler Stars

The aim of this Thesis is to investigate the dynamical evolution of Globular Clusters (GCs) by exploiting the properties of a dynamically-sensitive stellar population: Blue Straggler Stars (BSSs). These objects are ∼3 times more massive than the average in GCs, and their presence cannot be explained in terms of the standard evolution of single stars. This Thesis provides the determination of the physical properties (mass, temperature, radius, surface gravity) of BSSs along the entire extension of their sequence in the color-magnitude diagram, a study that confirms the large mass of these objects. Being more massive than the average, BSSs significantly suffer from the effects of dynamical friction, which makes them sink toward the cluster center. We demonstrated that the selection of BSSs at ultraviolet wavelengths guarantees the highest achievable level of completeness, and we used this approach to determine the BSS radial distribution in ∼30% of the entire Milky Way GC population. This allowed us to rank the host clusters in terms of the level of their internal dynamical evolution. The same approach applied to five GCs in the Large Magellanic Cloud not only demonstrated that the BSS radial distribution is a powerful dynamical indicator even in external galaxies, but also allowed us to show that the spread in core radius observed for the old GCs in the Large Magellanic Cloud is just the natural consequence of their internal dynamical evolution. We also pursued the search for double BSS sequence in M15 and NGC 1261. In M15, we found evidence for two distinct sequences of collisional BSSs that likely testify the occurrence of the core collapse and a subsequent core oscillation. Instead, in NGC 1261 we found only a hint of a double BSS sequence, the detectability of which is not as solid as for the other reported cases

Le Blue Straggler Stars e le popolazioni multiple in quattro ammassi globulari galattici

In questo elaborato viene presentato lo studio fotometrico di quattro ammassi globulari galattici. I target di questa Tesi fanno parte della HST UV Legacy Survey degli ammassi globulari galattici (Piotto et al. 2015). Nell'ambito di questa survey sono stati osservati, in modo omogeneo, 57 ammassi globulari galattici con il telescopio spaziale Hubble e la camera WFC3, in tre bande fotometriche ultraviolette e blu. Un dataset così composto è adatto a numerosi scopi, tra cui lo studio delle popolazioni calde come le BSS e delle popolazioni multiple. Sono stati selezionati quattro ammassi particolarmente popolosi e tra i più densi del campione, allo scopo di mettere a punto indicatori di evoluzione dinamica e comprendere il ruolo di quest'ultima sulle proprietà delle popolazioni multiple presenti nei sistemi selezionati. Lo studio dell'evoluzione dinamica è stato effettuato tramite la distribuzione radiale delle BSS (Blue Straggler Stars), che è stato dimostrato esserne un efficiente indicatore (Ferraro et al. 2012). I risultati ottenuti evidenziano chiaramente che tutti gli ammassi selezionati si trovano in fasi avanzate di evoluzione dinamica, come suggerito dall'alta densità che li caratterizza. Anche lo studio delle proprietà delle popolazioni multiple, ovvero sottopopolazioni con differenti abbondanze chimiche di elementi leggeri, la cui presenza è stata recentemente osservata negli ammassi globulari, è stato effettuato tramite lo studio della loro distribuzione radiale. Tra i quattro casi analizzati, soltanto M 15 ha mostrato una separazione significativa tra le distribuzioni radiali delle due popolazioni

Kinematic complexity around NGC 419: resolving the proper motion of the cluster, the Small Magellanic Cloud, and the Magellanic bridge

We present $\it{Hubble}$ $\it{Space}$ $\it{Telescope}$ proper motions in the direction of the star cluster NGC$\,$419 in the Small Magellanic Cloud. Because of the high precision of our measurements, for the first time it is possible to resolve the complex kinematics of the stellar populations located in the field, even along the tangential direction. In fact, the proper motions we measured allow us to separate cluster stars, which move on average with ($\mu_{\alpha}\cos\delta^{\rm NGC\,419}, \mu_{\delta}^{\rm NGC\,419}$) = ($+0.878\pm0.055$, $-1.246\pm0.048$) mas yr$^{-1}$, from those of the Small Magellanic Cloud and those belonging to a third kinematic feature that we recognise as part of the Magellanic Bridge. Resolving such a kinematic complexity enables the construction of decontaminated colour-magnitude diagrams, as well as the measurement of the absolute proper motion of the three separate components. Our study therefore sets the first steps towards the possibility of dynamically investigating the Magellanic system by exploiting the resolved kinematics of its stellar clusters.Comment: 9 pages, 9 figures, accepted for publication in MNRA

Extended Main-Sequence Turnoff and Red Clump in intermediate-age star clusters: A study of NGC 419

With the goal of untangling the origin of extended main-sequence turnoffs (eMSTOs) and extended red clumps (eRCs) in star clusters, in this work we present the study of the intermediate-age cluster NGC 419, situated along the Bridge of the Small Magellanic Cloud. To this aim, we analyzed multi-epoch, high angular resolution observations acquired with the Hubble Space Telescope for this dynamically young cluster, which enabled the determination of precise proper motions and therefore the assessment of the cluster membership for each individual star in the field of view. With this unprecedented information at hand, we first studied the radial distribution of kinematically selected member stars in different eMSTO subregions. The absence of segregation supports the rotation scenario as the cause for the turnoff color extension and disfavors the presence of a prolonged period of star formation in the cluster. A similar analysis on the eRC of NGC 419 confirms the absence of segregation, providing further evidence against an age spread, which is at odds with previous investigations. Even so, the currently available evolutionary models including stellar rotation fail at reproducing the two photometric features simultaneously. We argue that either shortcomings in these models or a different origin for the red clump feature, such as a nonstandard differential mass loss along the red giant branch phase, are the only way to reconcile our observational findings with theoretical expectations.Comment: 6 pages, 8 figures, Accepted for publication on A&

Blue Stragglers as tracers of the dynamical state of two clusters in the Small Magellanic Cloud: NGC 339 and NGC 419

The level of central segregation of Blue Straggler stars proved to be an excellent tracer of the dynamical evolution of old star clusters (the so-called "dynamical clock"), both in the Milky Way and in the Large Magellanic Cloud. The $A^{+}$ parameter, used to measure the Blue Stragglers degree of segregation, has in fact been found to strongly correlate with the parent cluster central relaxation time. Here we studied the Blue-Straggler population of two young stellar systems in the Small Magellanic Cloud, namely NGC 339 (which is 6 Gyr old) and NGC 419 (with an age of only 1.5 Gyr), in order to study their dynamical state. Thanks to multi-epoch, high angular resolution Hubble Space Telescope observations available for both clusters, we took advantage of the stellar proper motions measured in the regions of the two systems and we selected a population of likely cluster members, removing the strong contamination from Small Magellanic Cloud stars. This enabled us to study, with unprecedented accuracy, the radial distribution of Blue Stragglers in these two extragalactic clusters and to measure their dynamical age. As expected for such young clusters, we found that both systems are poorly evolved from the dynamical point of view, also fully confirming that the $A^{+}$ parameter is a sensitive "clock hand" even in the dynamically-young regime.Comment: 12 pages,11 figures, Accepted for publication by Ap

A new procedure for an effective management of geo-hydrological risks across the "Sentiero Verde-Azzurro" trail, Cinque Terre National Park, Liguria (North-Western Italy)

In recent years, Cinque Terre National Park, one of the most famous UNESCO sites in Italy, experienced a significant increase in tourist visits. This unique landscape is the result of the rough morphology of a small coastal basin with a very steep slope and a long-term human impact, mainly represented by anthropic terraces. This setting promotes the activation of numerous geo-hydrological instabilities, primarily related to heavy rainfall events that often affect this area. Currently, the main challenge for the administrators of Cinque Terre National Park is the correct maintenance of this environment along with the functional management of the hiking trail to ensure the safety of tourists. The definition of a methodology for effective management is mandatory for the sustainable administration of this unique site. We implement a new codified procedure based on the combined use of the Operative Monography and the Survey Form, focusing on the "Sentiero Verde-Azzurro" trail, for a proper description of the known landslides affecting the trail and the identification of damage and/or landslides activated by critical meteorological events. This guarantees effective geo-hydrological risk management, which is also applicable to other similar sites in a unique environmental and cultural heritage site such as Cinque Terre Park

Discovery of a double Blue Straggler sequence in M15: new insight into the core-collapse process

In this paper we report on the discovery of a double blue straggler star (BSS) sequence in the core of the core-collapsed cluster M15 (NGC 7078). We performed a detailed photometric analysis of the extremely dense core of the cluster using a set of images secured with the Advanced Camera for Survey in the High Resolution Channel mode on-board the Hubble Space Telescope. The proper combination of the large number of single frames in the near-UV (F220W), and blue (F435W) filters allowed us to perform a superb modeling of the Point Spread Function and an accurate deblending procedure. The Color-Magnitude diagram revealed the presence of two distinct parallel sequences of blue stragglers. In particular, the blue BSS sequence is characterized by the intriguing presence of two different branches. The first branch appears extremely narrow, it extends up to 2.5 magnitudes brighter than the cluster main-sequence turnoff (MS-TO) point, and it is nicely reproduced by a 2 Gyr-old collisional isochrone. The second branch extends up to 1.5 magnitudes from the MS-TO and it is reproduced by a 5.5 Gyr-old collisional isochrone. Our observations suggest that each of these branches is mainly constituted by a population of nearly coeval collisional BSS of different masses generated during two episodes of high collisional activity. We discuss the possibility that the oldest episode corresponds to the core-collapse event (occurred about 5.5 Gyr ago), while the most recent one (occurred about 2 Gyr ago) is associated with a core oscillation in the post-core collapse evolution. The discovery of these features provides further strong evidence in support of the connection between the BSS properties and GC dynamical evolution, and it opens new perspectives on the study of core-collapse and post core-collapse evolution.Comment: Accepted for publication on Ap

GMMA and Glycoconjugate Approaches Compared in Mice for the Development of a Vaccine against <i>Shigella flexneri</i> Serotype 6

Shigella infections are one of the top causes of diarrhea throughout the world, with Shigella flexneri being predominant in developing countries. Currently, no vaccines are widely available and increasing levels of multidrug-resistance make Shigella a high priority for vaccine development. The serotype-specific O-antigen moiety of Shigella lipopolysaccharide has been recognized as a key target for protective immunity, and many O-antigen based candidate vaccines are in development. Recently, the Generalized Modules for Membrane Antigens (GMMA) technology has been proposed as an alternative approach to traditional glycoconjugate vaccines for O-antigen delivery. Here, these two technologies are compared for a vaccine against S. flexneri serotype 6. Genetic strategies for GMMA production, conjugation approaches for linkage of the O-antigen to CRM197 carrier protein, and a large panel of analytical methods for full vaccine characterization have been put in place. In a head-to-head immunogenicity study in mice, GMMA induced higher anti-O-antigen IgG than glycoconjugate administered without Alhydrogel. When formulated on Alhydrogel, GMMA and glycoconjugate elicited similar levels of persistent anti-O-antigen IgG with bactericidal activity. Glycoconjugates are a well-established bacterial vaccine approach, but can be costly, particularly when multicomponent preparations are required. With similar immunogenicity and a simpler manufacturing process, GMMA are a promising strategy for the development of a vaccine against Shigella