Chemical and kinematical properties of Blue Straggler stars in Galactic globular clusters

Blue straggler stars (BSSs) are brighter and bluer (hotter) than the main-sequence (MS) turnoff and they are known to be more massive than MS stars.Two main scenarios for their formation have been proposed:collision-induced stellar mergers (COL-BSSs),or mass-transfer in binary systems (MT-BSSs).Depleted surface abundances of C and O are expected for MT-BSSs,whereas no chemical anomalies are predicted for COL-BSSs.Both MT- and COL-BSSs should rotate fast, but braking mechanisms may intervene with efficiencies and time-scales not well known yet,thus preventing a clear prediction of the expected rotational velocities.Within this context,an extensive survey is ongoing by using the multi-object spectrograph FLAMES@VLT,with the aim to obtain abundance patterns and rotational velocities for representative samples of BSSs in several Galactic GCs.A sub-population of CO-depleted BSSs has been identified in 47 Tuc,with only one fast rotating star detected.For this PhD Thesis work I analyzed FLAMES spectra of more than 130 BSSs in four GCs:M4,NGC 6397,M30 and ω Centauri.This is the largest sample of BSSs spectroscopically investigated so far.Hints of CO depletion have been observed in only 4-5 cases (in M30 and ω Centauri),suggesting either that the majority of BSSs have a collisional origin,or that the CO-depletion is a transient phenomenon.Unfortunately,no conclusions in terms of formation mechanism could be drawn in a large number of cases,because of the effects of radiative levitation. Remarkably,however,this is the first time that evidence of radiative levitation is found in BSSs hotter than 8200 K.Finally, we also discovered the largest fractions of fast rotating BSSs ever observed in any GCs:40% in M4 and 30% in ω Centauri.While not solving the problem of BSS formation,these results provide invaluable information about the BSS physical properties,which is crucial to build realistic models of their evolution.

The evolution of massive clumps in star forming regions

In this thesis two related arguments are investigated: - The first stages of the process of massive star formation, investigating the physical conditions and -properties of massive clumps in different evolutionary stages, and their CO depletion; - The influence that high-mass stars have on the nearby material and on the activity of star formation. I characterise the gas and dust temperature, mass and density of a sample of massive clumps, and analyse the variation of these properties from quiescent clumps, without any sign of active star formation, to clumps likely hosting a zero-age main sequence star. I briefly discuss CO depletion and recent observations of several molecular species, tracers of Hot Cores and/or shocked gas, of a subsample of these clumps. The issue of CO depletion is addressed in more detail in a larger sample consisting of the brightest sources in the ATLASGAL survey: using a radiative tranfer code I investigate how the depletion changes from dark clouds to more evolved objects, and compare its evolution to what happens in the low-mass regime. Finally, I derive the physical properties of the molecular gas in the photon-dominated region adjacent to the HII region G353.2+0.9 in the vicinity of Pismis 24, a young, massive cluster, containing some of the most massive and hottest stars known in our Galaxy. I derive the IMF of the cluster and study the star formation activity in its surroundings. Much of the data analysis is done with a Bayesian approach. Therefore, a separate chapter is dedicated to the concepts of Bayesian statistics.

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.

Different approaches to identify markers for meat quality and production traits in pigs: analysis of the transcriptome in post mortem skeletal muscle and investigation of candidate genes

Due to the growing attention of consumers towards their food, improvement of quality of animal products has become one of the main focus of research. To this aim, the application of modern molecular genetics approaches has been proved extremely useful and effective. This innovative drive includes all livestock species productions, including pork. The Italian pig breeding industry is unique because needs heavy pigs slaughtered at about 160 kg for the production of high quality processed products. For this reason, it requires precise meat quality and carcass characteristics. Two aspects have been considered in this thesis: the application of the transcriptome analysis in post mortem pig muscles as a possible method to evaluate meat quality parameters related to the pre mortem status of the animals, including health, nutrition, welfare, and with potential applications for product traceability (chapters 3 and 4); the study of candidate genes for obesity related traits in order to identify markers associated with fatness in pigs that could be applied to improve carcass quality (chapters 5, 6, and 7). Chapter three addresses the first issue from a methodological point of view. When we considered this issue, it was not obvious that post mortem skeletal muscle could be useful for transcriptomic analysis. Therefore we demonstrated that the quality of RNA extracted from skeletal muscle of pigs sampled at different post mortem intervals (20 minutes, 2 hours, 6 hours, and 24 hours) is good for downstream applications. Degradation occurred starting from 48 h post mortem even if at this time it is still possible to use some RNA products. In the fourth chapter, in order to demonstrate the potential use of RNA obtained up to 24 hours post mortem, we present the results of RNA analysis with the Affymetrix microarray platform that made it possible to assess the level of expression of more of 24000 mRNAs. We did not identify any significant differences between the different post mortem times suggesting that this technique could be applied to retrieve information coming from the transcriptome of skeletal muscle samples not collected just after slaughtering. This study represents the first contribution of this kind applied to pork. In the fifth chapter, we investigated as candidate for fat deposition the TBC1D1 [TBC1 (tre-2/USP6, BUB2, cdc16) gene. This gene is involved in mechanisms regulating energy homeostasis in skeletal muscle and is associated with predisposition to obesity in humans. By resequencing a fragment of the TBC1D1 gene we identified three synonymous mutations localized in exon 2 (g.40A>G, g.151C>T, and g.172T>C) and 2 polymorphisms localized in intron 2 (g.219G>A and g.252G>A). One of these polymorphisms (g.219G>A) was genotyped by high resolution melting (HRM) analysis and PCR-RFLP. Moreover, this gene sequence was mapped by radiation hybrid analysis on porcine chromosome 8. The association study was conducted in 756 performance tested pigs of Italian Large White and Italian Duroc breeds. Significant results were obtained for lean meat content, back fat thickness, visible intermuscular fat and ham weight. In chapter six, a second candidate gene (tribbles homolog 3, TRIB3) is analyzed in a study of association with carcass and meat quality traits. The TRIB3 gene is involved in energy metabolism of skeletal muscle and plays a role as suppressor of adipocyte differentiation. We identified two polymorphisms in the first coding exon of the porcine TRIB3 gene, one is a synonymous SNP (c.132T> C), a second is a missense mutation (c.146C> T, p.P49L). The two polymorphisms appear to be in complete linkage disequilibrium between and within breeds. The in silico analysis of the p.P49L substitution suggests that it might have a functional effect. The association study in about 650 pigs indicates that this marker is associated with back fat thickness in Italian Large White and Italian Duroc breeds in two different experimental designs. This polymorphisms is also associated with lactate content of muscle semimembranosus in Italian Large White pigs. Expression analysis indicated that this gene is transcribed in skeletal muscle and adipose tissue as well as in other tissues. In the seventh chapter, we reported the genotyping results for of 677 SNPs in extreme divergent groups of pigs chosen according to the extreme estimated breeding values for back fat thickness. SNPs were identified by resequencing, literature mining and in silico database mining. analysis, data reported in the literature of 60 candidates genes for obesity. Genotyping was carried out using the GoldenGate (Illumina) platform. Of the analyzed SNPs more that 300 were polymorphic in the genotyped population and had minor allele frequency (MAF) >0.05. Of these SNPs, 65 were associated (P<0.10) with back fat thickness. One of the most significant gene marker was the same TBC1D1 SNPs reported in chapter 5, confirming the role of this gene in fat deposition in pig. These results could be important to better define the pig as a model for human obesity other than for marker assisted selection to improve carcass characteristics.

Efficacia e sicurezza della profilassi anti-citomegalovirus rispetto alla strategia pre-sintomatica con valganciclovir in pazienti con trapianto di cuore trattati con everolimus o micofenolato

Il CMV è l’agente patogeno più frequente dopo trapianto (Tx) di cuore determinando sia sindromi cliniche organo specifiche sia un danno immunomediato che può determinare rigetto acuto o malattia coronarica cronica (CAV). I farmaci antivirali in profilassi appaiono superiori all’approccio pre-sintomatico nel ridurre gli eventi da CMV, ma l’effetto anti-CMV dell’everolimus (EVE) in aggiunta alla profilassi antivirale non è stato ancora analizzato. SCOPO DELLO STUDIO: analizzare l’interazione tra le strategie di profilassi antivirale e l’uso di EVE o MMF nell’incidenza di eventi CMV correlati (infezione, necessità di trattamento, malattia/sindrome) nel Tx cardiaco. MATERIALI E METODI: sono stati inclusi pazienti sottoposti a Tx cardiaco e trattati con EVE o MMF e trattamento antivirale di profilassi o pre-sintomatico. L’infezione da CMV è stata monitorata con antigenemia pp65 e PCR DNA. La malattia/sindrome da CMV è stato considerato l’endpoint principale. RISULTATI: 193 pazienti (di cui 10% D+/R-) sono stati inclusi nello studio (42 in EVE e 149 in MMF). Nel complesso, l’infezione da CMV (45% vs. 79%), la necessità di trattamento antivirale (20% vs. 53%), e la malattia/sindrome da CMV (2% vs. 15%) sono risultati significativamente più bassi nel gruppo EVE che nel gruppo MMF (tutte le P<0.01). La profilassi è più efficace nel prevenire tutti gli outcomes rispetto alla strategia pre-sintomatica nei pazienti in MMF (P 0.03), ma non nei pazienti in EVE. In particolare, i pazienti in EVE e strategia pre-sintomatica hanno meno infezioni da CMV (48 vs 70%; P=0.05), e meno malattia/sindrome da CMV (0 vs. 8%; P=0.05) rispetto ai pazienti in MMF e profilassi. CONCLUSIONI: EVE riduce significamene gli eventi correlati al CMV rispetto al MMF. Il beneficio della profilassi risulta conservato solo nei pazienti trattati con MMF mentre l’EVE sembra fornire un ulteriore protezione nel ridurre gli eventi da CMV senza necessità di un estensivo trattamento antivirale.

Modeling systems and vis/NIR device to improve peach and nectarine pre and post-harvest fruit maturity management

During the last decade peach and nectarine fruit have lost considerable market share, due to increased consumer dissatisfaction with quality at retail markets. This is mainly due to harvesting of too immature fruit and high ripening heterogeneity. The main problem is that the traditional used maturity indexes are not able to objectively detect fruit maturity stage, neither the variability present in the field, leading to a difficult post-harvest management of the product and to high fruit losses. To assess more precisely the fruit ripening other techniques and devices can be used. Recently, a new non-destructive maturity index, based on the vis-NIR technology, the Index of Absorbance Difference (IAD), that correlates with fruit degreening and ethylene production, was introduced and the IAD was used to study peach and nectarine fruit ripening from the “field to the fork”. In order to choose the best techniques to improve fruit quality, a detailed description of the tree structure, of fruit distribution and ripening evolution on the tree was faced. More in details, an architectural model (PlantToon®) was used to design the tree structure and the IAD was applied to characterize the maturity stage of each fruit. Their combined use provided an objective and precise evaluation of the fruit ripening variability, related to different training systems, crop load, fruit exposure and internal temperature. Based on simple field assessment of fruit maturity (as IAD) and growth, a model for an early prediction of harvest date and yield, was developed and validated. The relationship between the non-destructive maturity IAD, and the fruit shelf-life, was also confirmed. Finally the obtained results were validated by consumer test: the fruit sorted in different maturity classes obtained a different consumer acceptance. The improved knowledge, leaded to an innovative management of peach and nectarine fruit, from “field to market”.

Gestione pre, intra e post-operatoria del cane sottoposto ad ipofisectomia transfenoidale

L’approccio chirurgico agli adenomi ipofisari ACTH secernenti è la terapia d’elezione nell’uomo. L’ipofisectomia transfenoidale è invece una tecnica poco diffusa in ambito veterinario. La terapia più diffusa nel cane con ipercortisolismo ipofisi dipendente (PDH) è di tipo medico e prevede la somministrazione di farmaci inibitori della sintesi del cortisolo. Gli adenomi ipofisari possono aumentare di volume e determinare una conseguente sintomatologia neurologica; in questi casi le uniche opzioni terapeutiche sono rappresentate dall’asportazione chirurgica della neoplasia e dalla radioterapia. Nella presente tesi vengono descritti 8 interventi di ipofisectomia transfenoidale effettuati su 7 cani con macroadenoma ipofisario presso il Dipartimento di Scienze Mediche Veterinarie dell’Università di Bologna. La difficoltà maggiore per il chirurgo è rappresentata dalla localizzazione della fossa ipofisaria rispetto ai punti di repere visibile in tomografia computerizzata o in risonanza magnetica nucleare, oltre ai problemi di sanguinamento durante la rimozione della neoplasia. Nel periodo post-operatorio maggiori complicazioni si riscontrano in soggetti con adenomi ipofisari di maggiori dimensioni. Al contrario, in presenza di adenomi di dimensioni più contenute, la ripresa post-operatoria risulta più rapida e il tasso di successo maggiore. Al fine di poter eseguire nel cane l’exeresi mirata della sola neoplasia ipofisaria, al pari di quanto avviene nell’uomo, è stato condotto uno studio sulla tomografia computerizzata (TC) in 86 cani con PDH. Il protocollo TC non ha tuttavia permesso di individuare con precisione la posizione della neoplasia per guidare il chirurgo nella sua rimozione. In due casi riportati nel presente lavoro si è verificata una recidiva della neoplasia ipofisaria. In un soggetto si è optato per il reintervento, mentre nell’altro caso per la radioterapia. Entrambe le opzioni hanno garantito una buona qualità di vita per più di un anno dall’intervento terapeutico. Questi casi clinici dimostrano come il reintervento e la radioterapia possano essere considerate valide opzioni in caso di recidiva.