Spatial features of non-thermal SZ effect in galaxy clusters

We investigate the spatial behaviour of the total comptonization parameter $y_{tot}$ evaluated for a galaxy cluster containing two population of electrons: the thermal population, with energy around some KeV and whose trace is evident in the X-ray emission of the ICM (Intra-Cluster Medium), and the relativistic population, which give rise to the radio halo emission found in several clusters of galaxies. We present the first results obtained from our analysis showing that there are remarkable features in such spatial trend, which might throw a new light in understanding the cluster internal processes.Comment: 4 pages, 1 figure, to appear in the proceedings of the 2k1bc workshop ""Experimental comsology @ millimetre wavelengths", july 9-12 2001, Breuil-Cervinia, Ital

The Non-Thermal Sunyaev-Zel'dovich Effect in Clusters of Galaxies

In this paper we provide a general derivation of the non-thermal (as well as of the thermal) SZ effect in galaxy clusters which is exact in the Thomson limit to any approximation order in the optical depth. Such a general derivation is obtained using the full relativistic formalism and overcoming the limitations of the Kompaneets and of the single scattering approximations. To have a consistent description of the SZ effect in clusters containing non-thermal phenomena, we also evaluate in a consistent way - for the first time - the total SZ effect produced by a combination of thermal and non-thermal electron populations residing in the same environment, like is the case in radio-halo clusters. We discuss both the spectral and the spatial features of the total SZ effect and we provide specific predictions for a well studied radio-halo cluster like A2163. We also discuss the overall SZ effect produced by a combination of different thermal populations residing in the cluster atmosphere. In this context, we discuss how the combined observations of the thermal and non-thermal SZ effect provide constraints on the spectrum of the relativistic electron population and, in turn, on the presence and on the origin of non-thermal phenomena (radio-halo, hard X-ray, EUV excesses) occurring in galaxy clusters

Ethnic Bullying Victimization in Italy: The Role of Acculturation Orientation for Ethnic Minority Adolescents With Differing Citizenship Statuses

This study examines the role of acculturation orientation toward home and host countries in ethnic bullying victimization, by considering citizenship status and taking into account social withdrawal. Within a larger school project with middle and high school students, we analyzed data on 252 adolescents from immigrant backgrounds: 71 born abroad without Italian citizenship (Males = 71.4%; mean age = 13.98, SD = 1.7); 96 born in Italy to immigrant parents and without Italian citizenship (Males = 58.3%; mean age = 13.26, SD = 1.6); and 85 Italian citizens born in Italy with an immigrant parent (Males = 54.7%; mean age = 13.12, SD = 1.5). At the univariate level we found that the group of adolescents born abroad with foreign parents showed significantly higher levels of ethnic victimization compared to the group of adolescents born in Italy with an Italian parent. The latter also reported a significantly higher mean in Acculturation Orientation toward their Host Country (i.e., Italy) compared to the other two groups. Looking at the processes working within each group, we found differences in the patterns of association between acculturation orientation and ethnic bullying victimization. Specifically, we found a significant and positive association between acculturation orientation toward the home country and ethnic victimization in the two groups of adolescents born in Italy, while acculturation orientation toward the host country seems to be a protective factor only for adolescents with Italian citizenship. Acculturation orientation does not play any role in ethnic victimization for the first generation of immigrants, while for this group we found a stronger positive effect of Social Withdrawal. Citizenship status appears to be a good indicator of belonging to an ethnic minority group with a background of immigration: it seems to catch specific processes in ethnic bullying victimization. © Copyright © 2020 Palladino, Nappa, Zambuto and Menesini

Hypervelocity Star Candidates in the SEGUE G & K Dwarf Sample

We present 20 candidate hypervelocity stars from the Sloan Extension for Galactic Understanding and Exploration (SEGUE) G and K dwarf samples. Previous searches for hypervelocity stars have only focused on large radial velocities; in this study we also use proper motions to select the candidates. We determine the hypervelocity likelihood of each candidate by means of Monte Carlo simulations, considering the significant errors often associated with high proper motion stars. We find that nearly half of the candidates exceed their escape velocities with at least 98% probability. Every candidate also has less than a 25% chance of being a high-velocity fluke within the SEGUE sample. Based on orbits calculated using the observed six-dimensional positions and velocities, few, if any, of these candidates originate from the Galactic center. If these candidates are truly hypervelocity stars, they were not ejected by interactions with the Milky Way's supermassive black hole. This calls for a more serious examination of alternative hypervelocity-star ejection scenarios.Comment: 8 pages, 5 figures, published in ApJ, this version includes all figures as intende

Impactos das mudanças climáticas sobre a distribuição espacial da podridão cinzenta em videira no Brasil.

Resumo: A podridão cinzenta, causada pelo fungo Botryotinia fuckeliana (Botrytis cinerea), existente em praticamente todos os vinhedos do mundo, causa sérias reduções na qualidade e na quantidade de uva produzida. O estudo teve como objetivo avaliar os impactos das mudanças climáticas na favorabilidade de ocorrência da podridão cinzenta da videira no Brasil. Foram utilizadas informações de temperatura média e período de molhamento foliar do período de referência (1961 ? 1990) e do futuro (2011 ? 2040, 2041 ? 2070 e 2071 ? 2100) para o Brasil, dos cenários A2 e B1, organizadas no banco de dados em Sistema de Informações Geográficas (SIG) Idrisi 32. A favorabilidade foi obtida aplicando-se equações lógicas, de acordo com as condições e restrições de período de molhamento foliar e temperatura média, resultando em mapas de distribuição espacial da podridão cinzenta no Brasil. De modo geral, é esperado um quadro positivo para o futuro, pois as áreas onde a condição para o desenvolvimento da doença era muito favorável diminuem, e as áreas de condição desfavorável apresentam um aumento principalmente durante o inverno. Abstract; The gray mold, caused by the fungus Botryotinia fuckeliana (Botrytis cinerea), which exists in almost all vineyards in the world, causes serious reductions in quality and quantity of grapes produced. The study aimed to evaluate the impacts of climate change on the favorability of occurrence of gray rot of grapevine in Brazil. Information was collected from average temperature and leaf wetness of the reference period (1961 - 1990) and future (2011 - 2040, 2041 - 2070 and 2071 - 2100) for Brazil, organized in the database in a Geographic Information System (GIS) Idrisi 32. The favorability was obtained by applying logic equations, according to the conditions and restrictions of leaf wetness and average temperature, resulting in maps of spatial distribution of gray mold in Brazil. In general, it can be expected a positive picture for the future, because the areas where the condition for the development of the disease was very favorable decreased, and the areas of unfavorable condition showed an increase mainly during the winter

Cosmic Microwave Background Temperature at Galaxy Clusters

We have deduced the cosmic microwave background (CMB) temperature in the Coma cluster (A1656, $z=0.0231$), and in A2163 ($z=0.203$) from spectral measurements of the Sunyaev-Zel'dovich (SZ) effect over four passbands at radio and microwave frequencies. The resulting temperatures at these redshifts are $T_{Coma} = 2.789^{+0.080}_{-0.065}$ K and $T_{A2163} = 3.377^{+0.101}_{-0.102}$ K, respectively. These values confirm the expected relation $T(z)=T_{0}(1+z)$, where $T_{0}= 2.725 \pm 0.002$ K is the value measured by the COBE/FIRAS experiment. Alternative scaling relations that are conjectured in non-standard cosmologies can be constrained by the data; for example, if $T(z) = T_{0}(1+z)^{1-a}$ or $T(z)=T_{0}[1+(1+d)z]$, then $a=-0.16^{+0.34}_{-0.32}$ and $d = 0.17 \pm 0.36$ (at 95% confidence). We briefly discuss future prospects for more precise SZ measurements of $T(z)$ at higher redshifts.Comment: 13 pages, 1 figure, ApJL accepted for publicatio