Lyapunov functions for a non-linear model of the X-ray bursting of the microquasar GRS 1915+105

This paper introduces a biparametric family of Lyapunov functions for a non-linear mathematical model based on the FitzHugh-Nagumo equations able to reproduce some main features of the X-ray bursting behaviour exhibited by the microquasar GRS 1915+105. These functions are useful to investigate the properties of equilibrium points and allow us to demonstrate a theorem on the global stability. The transition between bursting and stable behaviour is also analyzed.Comment: Published on International Journal of Non-Linear Mechanics, vol. 88, pp. 142-14

The complex time behaviour of the microquasar GRS 1915+105 in the \rho-class observed with BeppoSAX. III: The hard X-ray delay and limit cycle mapping

The microquasar GRS1915+105 was observed by BeppoSAX in October 2000 for about ten days while the source was in \rho-mode, which is characterized by a quasi-regular type I bursting activity. This paper presents a systematic analysis of the delay of the hard and soft X-ray emission at the burst peaks. The lag, also apparent from the comparison of the [1.7-3.4] keV light curves with those in the [6.8-10.2] keV range, is evaluated and studied as a function of time, spectral parameters, and flux. We apply the limit cycle mapping technique, using as independent variables the count rate and the mean photon rate. The results using this technique were also cross-checked using a more standard approach with the cross-correlation methods. Data are organized in runs, each relative to a continuous observation interval. The detected hard-soft delay changes in the course of the pointing from about 3 s to about 10 s and presents a clear correlation with the baseline count rate.Comment: accepted for publication in A&

Gli uccelli delle isole circumsiciliane

Gli autori sintetizzano tutte le informazioni bibliografiche e inedite sulle specie che sino al 30 agosto 2015 sono state contattate almeno una volta nelle 14 isole circumsiciliane (Eolie, Ustica, Egadi, Pantelleria e Pelagie), confrontando alla fine la lista complessiva con quella delle isole Maltesi. In totale sono ad oggi note 434 specie (isole Maltesi incluse); molte di esse hanno mostrato nel corso dei secoli una notevole capacità di colonizzazione, fluttuando nel tempo o addirittura estinguendosi e ricolonizzando alcune isole. Questi piccoli territori in mezzo al mare rappresentano ottimi siti di controllo dell’andamento delle migrazioni nel corso dei decenni; alcune specie hanno chiaramente cambiato il loro status rispetto al passato, aumentando o diminuendo. Nel corso di circa 15 anni in alcune di queste isole (Ustica, Marettimo, Lampedusa e Linosa) sono stati condotti dei campi di inanellamento sia primaverili sia autunnali che hanno permesso di inanellare 102.208 uccelli, in gran parte Passeriformes; ciò ha consentito di raccogliere una notevole mole di dati sulle strategie migratorie, che vengono qui brevemente presentati. Le piccole isole sono davvero importanti per gli uccelli migratori transahariani, che devono sostare durante i loro lunghi viaggi per recuperare energie; la disponibilità di risorse sotto forma di frutti selvatici o di insetti (a seconda delle specie) consente a queste masse di migratori di continuare il loro viaggio. La conservazione degli uccelli è dettata dalla Direttiva Uccelli e l’istituzione delle Zone di Protezione Speciale ha proprio lo scopo di salvaguardare alcune specie in determinati territori. Questo è un impegno preso da parte di tutti i Paesi dell’Unione Europea, proprio perché le popolazioni di uccelli non conoscono confini amministrativi e la loro tutela va al di là delle competenze e degli interessi di un singolo Paese. Per quanto riguarda le specie nidificanti, è risultata un’elevata correlazione negativa (r=-0,746), altamente significativa (P=0,002) tra la capacità dispersiva media delle specie e la superficie in km2 delle isole. Le specie con minore capacità dispersiva hanno colonizzato le isole di maggiori dimensioni, ma non quelle più piccole; questo con molta probabilità dipende dalla eterogeneità ambientale, a sua volta legata alla dimensione delle isole ed alla loro posizione geografica. Nel caso delle isole circumsiciliane, sembra che non sia tanto la distanza dalla costa a determinare il numero di specie, quanto le condizioni ambientali e la posizione geografica; indubbiamente la posizione tirrenica delle isole settentrionali rappresenta un vantaggio per la presenza di habitat differenziati e la conseguente colonizzazione di specie ad essi legate, mentre la posizione meridionale, influenzata dall’aridità africana, riduce alcune possibilità colonizzatrici da parte di alcune specie di uccelli e rende altresì problematica la stessa esistenza di habitat diversificati. Il numero delle specie nidificanti in un’isola è variabile nel tempo, essendovi specie che vi nidificano in modo irregolare. La correlazione area/N° specie nelle isole circumsiciliane è pari a 0,58, ma se si esclude l’isola di Pantelleria, sale a 0,86; essa è pari a 0,92 per le sole isole settentrionali (Eolie, Ustica ed Egadi), mentre risulta 0,99 per le sole tre isole meridionali del Canale di Sicilia.Authors summarize all bibliographic and unpublished information on bird species that have been detected at least one time up to 30th August 2015 in the 14 circum-sicilian islands (Eolian, Ustica, Egadi, Pantelleria and Pelagian Is.). The Appendix 1 compares overall lists with that of the Maltese Is., also lying in the Sicilian waters. On the whole, 434 species are known till now (Maltese Is. included); many of them showed a high colonizing capacity along the centuries, fluctuating or even becoming extinct and re-colonising some islands. These small territories in the middle of the Mediterranean sea are very good check-control sites of long-term migration trend; compared to the past, some species changed their status, increasing or declining. Additionally, during the last 15 years in some of these islands (Ustica, Marettimo, Lampedusa and Linosa) bird ringing activity has been carried out, both in spring and in autumn; it allowed to ring 102,208 birds, mainly Passeriformes; this opportunity allowed to collect a remarkable amount of data on migration strategy, here presented. The small islands are very important stop-over sites for transsaharan migratory birds, that must rest during their long journey to recover fuel in the form of fat; the availability of natural resources, such as wild fruits or insects, allows these masses of migrant birds to continue their trip. The conservation of birds has been established by the Bird Directive and the institution of Zones of Special Protection has the aim to safeguard some species in some territories. This agreement was signed by all countries of the EU, because bird populations do not know administrative borders and their conservation lies beyond the interests and authorities of a single country. Concerning breeding birds, a high negative correlation (r=-0.746, P=0.002) has been found between the average dispersal power of species and the area in km2 of islands. Species with minor dispersal power colonized the biggest but not the smallest islands; this, very probably depended on habitat heterogeneity of islands, in turn linked to the size of them and to the geographical position, more than to the distance from the continental land. Tyrrhenian position of northern islands is certainly an advantage for the presence of diversified habitats and birds inhabiting them, whereas southern position of Pantelleria and Pelagian Is., as well as Maltese Is., affected by African dryness, decreases colonizing probabilities of some bird species and the same existence of diversified habitats. The number of breeding species in each island varied along the time and some species bred irregularly. The correlation area/No. species in the islands surrounding Sicily resulted to be 0.58, but if we exclude Pantelleria Is., it grows to 0.86; besides, it grows to 0.92 if we consider only northern islands (Eolian, Ustica and Egadi Is.), and to 0.99 if we consider only southern islands

Timing analysis of 10-day long BeppoSAX observation of GRS 1915+105 in its ρ class

Published online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=6

Rainbow trout (Oncorhynchus mykiss, Walbaum 1792) develop a more robust body shape under organic rearing

Prolonged exposure to captive conditions has led to the development of a rainbow trout ‘farmed’ pheno- type, which is different from that of wild trout. Selec- tion for desirable productive traits in hatcheries has resulted in the development of some morphological traits that are maladaptive in nature. The recent development of organic aquaculture, guided by the well-being of the fish, could potentially produce a new farmed phenotype that would be more adaptive in nature. In this study, rainbow trout reared in intensive and organic farms were compared by means of shape analysis, to detect patterns of shape variation associated with rearing environment. The results of this study highlight a significant effect of the rearing method on rainbow trout shape: organi- cally reared trout showed a higher body profile, in particular in the head and trunk regions, shorter median fins and a deeper caudal peduncle. A combined effect of density and habitat complexity could have contributed to the observed shape differences: in organic rearing systems, lower densi- ties and steady water could increase territoriality and aggressive interactions, promoting body designs more functional in rapid attacks and escapes

Modulating the WNT pathway in Drosophila models of Cornelia de Lange Syndrome

Cornelia de Lange syndrome (CdLS) is a rare genetic disorder affecting neurodevelopment and the gastrointestinal and musculoskeletal systems. CdLS is caused by mutations within NIPBL, SMC1A, SMC3, RAD21, HDAC8 and BRD4 genes. These genes codify for the cohesin complex (or associated proteins), a multiprotein structure playing a role in chromatid adhesion, DNA repair and gene expression regulation. Our laboratory has shown that a strong correlation exists between cohesin complex function and WNT signalling, an intracellular pathway involved in regulation of expression of several genes controlling cell division and embryonic development. Recently, it has been observed that in nipblb- and smc1a-loss-of-function zebrafish embryos, in NIPBL- and SMC1A- mutated patient fibroblasts and in CdLS murine neural stem cells (NSCs) similar patterns of canonical WNT pathway alterations and cyclinD1 downregulation are present. Indeed, zebrafish embryos adverse phenotype was rescued by chemical activation of the WNT pathway. Drosophila melanogaster is an inexpensive model to study CdLS and to screen in vivo for therapeutic compounds. Therefore, we have used flies\u2019 strains mutated in nipped-B and hdac3 genes (respectively NIPBL and HDAC8 in humans) for assessing the existing correlation between cohesin complex and WNT pathway. Moreover, we have selected D. melanogaster mutants to screen for chemicals that revert the CdLS associated-phenotypes efficiently. In particular, we have tested WNT activators in order to investigate which effects they have on the mutated flies, assessing body weight and changes in brain structures (i.e. mushroom bodies) and possibly select compounds to test on vertebrate models. Funding: This work has been supported by Fondazione Cariplo, grant 2015-0783 to Valentina Massa

A new FSA approach for in situ γ\gamma-ray spectroscopy

An increasing demand of environmental radioactivity monitoring comes both from the scientific community and from the society. This requires accurate, reliable and fast response preferably from portable radiation detectors. Thanks to recent improvements in the technology, $\gamma$-spectroscopy with sodium iodide scintillators has been proved to be an excellent tool for in-situ measurements for the identification and quantitative determination of $\gamma$-ray emitting radioisotopes, reducing time and costs. Both for geological and civil purposes not only $^{40}$K, $^{238}$U, and $^{232}$Th have to be measured, but there is also a growing interest to determine the abundances of anthropic elements, like $^{137}$Cs and $^{131}$I, which are used to monitor the effect of nuclear accidents or other human activities. The Full Spectrum Analysis (FSA) approach has been chosen to analyze the $\gamma$-spectra. The Non Negative Least Square (NNLS) and the energy calibration adjustment have been implemented in this method for the first time in order to correct the intrinsic problem related with the $\chi ^2$ minimization which could lead to artifacts and non physical results in the analysis. A new calibration procedure has been developed for the FSA method by using in situ $\gamma$-spectra instead of calibration pad spectra. Finally, the new method has been validated by acquiring $\gamma$-spectra with a 10.16 cm x 10.16 cm sodium iodide detector in 80 different sites in the Ombrone basin, in Tuscany. The results from the FSA method have been compared with the laboratory measurements by using HPGe detectors on soil samples collected in the different sites, showing a satisfactory agreement between them. In particular, the $^{137}$Cs isotopes has been implemented in the analysis since it has been found not negligible during the in-situ measurements.Comment: accepted by Science of Total Environment: 8 pages, 10 figures, 3 table

The Discordance of Mass-Loss Estimates for Galactic O-Type Stars

We have determined accurate values of the product of the mass-loss rate and the ion fraction of P^{4+}, Mdot q(P^{4+}), for a sample of 40 Galactic O-type stars by fitting stellar-wind profiles to observations of the P V resonance doublet obtained with FUSE, ORFEUS/BEFS, and Copernicus. When P^{4+} is the dominant ion in the wind, Mdot q(P^{4+}) approximates the mass-loss rate to within a factor of 2. Theory predicts that P^{4+} is the dominant ion in the winds of O7-O9.7 stars, though an empirical estimator suggests that the range from O4-O7 may be more appropriate. However, we find that the mass-loss rates obtained from P V wind profiles are systematically smaller than those obtained from fits to Halpha emission profiles or radio free-free emission by median factors of about 130 (if P^{4+} is dominant between O7 and O9.7) or about 20 (if P^{4+} is dominant between O4 and O7). These discordant measurements can be reconciled if the winds of O stars in the relevant temperature range are strongly clumped on small spatial scales. We use a simplified two-component model to investigate the volume filling factors of the denser regions. This clumping implies that mass-loss rates determined from "density squared" diagnostics have been systematically over-estimated by factors of 10 or more, at least for a subset of O stars. Reductions in the mass-loss rates of this size have important implications for the evolution of massive stars and quantitative estimates of the feedback that hot-star winds provide to their interstellar environments.Comment: 26 pages, 4 figures; accepted for publication in Ap