A spectroscopic and photometric study of stellar populations in a sample of clusters in the Magellanic Clouds

This Ph.D. Thesis has been carried out in the framework of a long-term and large project devoted to describe the main photometric, chemical, evolutionary and integrated properties of a representative sample of Large and Small Magellanic Cloud (LMC and SMC respectively) clusters. The globular clusters system of these two Irregular galaxies provides a rich resource for investigating stellar and chemical evolution and to obtain a detailed view of the star formation history and chemical enrichment of the Clouds. The results discussed here are based on the analysis of high-resolution photometric and spectroscopic datasets obtained by using the last generation of imagers and spectrographs. The principal aims of this project are summarized as follows: • The study of the AGB and RGB sequences in a sample of MC clusters, through the analysis of a wide near-infrared photometric database, including 33 Magellanic globulars obtained in three observing runs with the near-infrared camera SOFI@NTT (ESO, La Silla). • The study of the chemical properties of a sample of MCs clusters, by using optical and near-infrared high-resolution spectra. 3 observing runs have been secured to our group to observe 9 LMC clusters (with ages between 100 Myr and 13 Gyr) with the optical high-resolution spectrograph FLAMES@VLT (ESO, Paranal) and 4 very young (<30 Myr) clusters (3 in the LMC and 1 in the SMC) with the near-infrared high-resolution spectrograph CRIRES@VLT. • The study of the photometric properties of the main evolutive sequences in optical Color- Magnitude Diagrams (CMD) obtained by using HST archive data, with the final aim of dating several clusters via the comparison between the observed CMDs and theoretical isochrones. The determination of the age of a stellar population requires an accurate measure of the Main Sequence (MS) Turn-Off (TO) luminosity and the knowledge of the distance modulus, reddening and overall metallicity. For this purpose, we limited the study of the age just to the clusters already observed with high-resolution spectroscopy, in order to date only clusters with accurate estimates of the overall metallicity.

Studio genetico ed epidemiologico su Erysiphe necator agente eziologico dell'Oidio della vite

The objective was to analyse population structure and to determine genetic diversity of Erysiphe necator (syn. Uncinula necator) populations obtained from some vineyards located in the South-East Po valley (Italy). Powdery mildew is one of the most important fungal diseases of grapes (Vitis vinifera L.) throughout the world. The causal agent is the haploid, heterothallic ascomycete E. necator. It is an obligate biotrophic fungus and it can be found only on green organs of plants belonging to the family Vitaceae. For this pathogen, two sympatric populations (groups A and B) have been described in Europe and Australia. The two genetic groups differ at multiple genetic loci and previous studies reported a lack of interfertility among isolates of the two groups. There are now several well documented examples of plant pathogen species, such as Leptosphaeria maculans, Gaeumannomyces graminis var. tritici, Botrytis cinerea and Erysiphe syringae, which are indeed composed of genetically differentiated clades, that have led to the description of new groups or even new species. Several studies have suggested that genetic E. necator group A and B correlated with ecological features of the pathogen; some researchers proposed that group A isolates over-winter as resting mycelium within dormant buds, and in spring originate infected shoots, known as Flag shoots, while group B isolates would survive as ascospores in overwintering cleistothecia. However, the association between genetic groups and mode of over-wintering has been challenged by recent studies reporting that flag-shoot may be originated indifferently by group A or group B isolate. Previous studies observed a strong association between the levels of disease severity at the end of the growing season and the initial compositions of E. necator populations in commercial vineyards. The frequencies of E. necator genetic groups vary considerably among vineyards, and the two groups may coexist in the same vineyard. This finding suggests that we need more information on the genetics and epidemiology of E. necator for optimize the crop management In this study we monitored E. necator populations in different vineyards in Emilia – Romagna region (Italy), where the pathogen overwinters both as flagshoots and as cleistothecia. During the grape growing season, symptomatic leaves were sampled early in the growing season and both leaves and berries later during the epidemic growth of the disease. From each sample, single-conidial isolate was obtained. Each isolates was grown on V. vinifera leaf cv. Primitivo and after harvesting the mycelium, the DNA was purified and used as template for PCR amplification with SCAR primers (Sequences Characterised Amplified Region ), -tubulin, IGS sequences and Microsatellite markers (SSR). Amplified DNA from b-tubulin and IGS loci was digested with AciI and XhoI restriction enzymes, respectively, to show single-nucleotide polymorphisms specific for the two genetic groups. The results obtained indicated that SCAR primers are not useful to study the epidemiology. of E. necator conversely the b-tubulin IGS sequences and SSR. Summarize the results obtained with b-tubulin, IGS sequences, in treated vineyards we have found individuals of group B along all grape growing season, whereas in the untreated vineyard individuals of the two genetic groups A and B coexisted throughout the season, with no significant change of their frequency. DNA amplified from ascospores of single cleistothecia showed the presence of markers diagnostic for either groups A and B and were seldom observed also the coexistence of both groups within a claistothecium. These results indicate that individuals of the two groups mated in nature and were able to produced ascospores. With SSR we showed the possibility of recombination between A and B groups in field isolates. During winter, cleistothecia were collected repeatedly in the same vineyards sampling leaves fallen on ground, exfoliating bark from trunks, and from soil. From each substrate, was assess the percentage of cleistothecia containing viable ascospores. Our results confirmed that cleisthotecia contained viable ascospores, therefore they have the potential to be an additional and important source of primary inoculum in Emilia-Romagna vineyards.

Homogeneous analysis of a sample of Open Clusters in the context of the BOCCE project and the Gaia-ESO Survey

The open clusters (OC) are gravitationally bound systems of a few tens or hundreds of stars. In our Galaxy, the Milky Way, we know about 3000 open clusters, of very different ages in the range of a few millions years to about 9 Gyr. OCs are mainly located in the Galactic thin disc, with distances from the Galactic centre in the range 4-22 kpc and a height scale on the disc of about 200 pc. Their chemical properties trace those of the environment in which they formed and the metallicity is in the range -0.5<[Fe/H]<+0.5 dex. Through photometry and spectroscopy it is possible to study relatively easily the properties of the OCs and estimate their age, distance, and chemistry. For these reasons they are considered primary tracers of the chemical properties and chemical evolution of the Galactic disc. The main subject of this thesis is the comprehensive study of several OCs. The research embraces two different projects: the Bologna Open Cluster Chemical Evolution project (BOCCE) and the Gaia-ESO Survey. The first is a long-term programme, aiming at studying the chemical evolution of the Milky Way disc by means of a homogeneous sample of OCs. The latter is a large public spectroscopy survey, conducted with the high-resolution spectrograph FLAMES@VLT and targeting about 10^5 stars in different part of the Galaxy and 10^4 stars in about 100 OCs. The common ground between the two projects is the study of the properties of the OCs as tracers of the disc's characteristics. The impressive scientific outcome of the Gaia-ESO Survey and the unique framework of homogeneity of the BOCCE project can propose, especially once combined together, a much more accurate description of the properties of the OCs. In turn, this will give fundamental constraints for the interpretation of the properties of the Galactic disc.