Investigation of the midgut structure and ultrastructure in Cimex lectularius and Cimex pipistrelli (Hemiptera, Cimicidae)

Cimicidae are temporary ectoparasites, which means that they cannot obtain food continuously. Both Cimex species examined here, Cimex lectularius (Linnaeus 1758) and Cimex pipistrelli (Jenyns 1839), can feed on a non-natal host, C. lectularius from humans on bats, C. pipistrelli on humans, but never naturally. The midgut of C. lectularius and C. pipistrelli is composed of three distinct regions—the anterior midgut (AMG), which has a sack-like shape, the long tube-shaped middle midgut (MMG), and the posterior midgut (PMG). The different ultrastructures of the AMG, MMG, and PMG in both of the species examined suggest that these regions must fulfill different functions in the digestive system. Ultrastructural analysis showed that the AMG fulfills the role of storing food and synthesizing and secreting enzymes, while the MMG is the main organ for the synthesis of enzymes, secretion, and the storage of the reserve material. Additionally, both regions, the AMG and MMG, are involved in water absorption in the digestive system of both Cimex species. The PMG is the part of the midgut in which spherites accumulate. The results of our studies confirm the suggestion of former authors that the structure of the digestive tract of insects is not attributed solely to diet but to the basic adaptation of an ancestor

The PLATO 2.0 mission

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses fundamental questions such as: How do planetary systems form and evolve? Are there other systems with planets like ours, including potentially habitable planets? The PLATO 2.0 instrument consists of 34 small aperture telescopes (32 with 25 s readout cadence and 2 with 2.5 s candence) providing a wide field-of-view (2232 deg 2) and a large photometric magnitude range (4-16 mag). It focusses on bright (4-11 mag) stars in wide fields to detect and characterize planets down to Earth-size by photometric transits, whose masses can then be determined by ground-based radial-velocity follow-up measurements. Asteroseismology will be performed for these bright stars to obtain highly accurate stellar parameters, including masses and ages. The combination of bright targets and asteroseismology results in high accuracy for the bulk planet parameters: 2 %, 4-10 % and 10 % for planet radii, masses and ages, respectively. The planned baseline observing strategy includes two long pointings (2-3 years) to detect and bulk characterize planets reaching into the habitable zone (HZ) of solar-like stars and an additional step-and-stare phase to cover in total about 50 % of the sky. PLATO 2.0 will observe up to 1,000,000 stars and detect and characterize hundreds of small planets, and thousands of planets in the Neptune to gas giant regime out to the HZ. It will therefore provide the first large-scale catalogue of bulk characterized planets with accurate radii, masses, mean densities and ages. This catalogue will include terrestrial planets at intermediate orbital distances, where surface temperatures are moderate. Coverage of this parameter range with statistical numbers of bulk characterized planets is unique to PLATO 2.0. The PLATO 2.0 catalogue allows us to e.g.: - complete our knowledge of planet diversity for low-mass objects, - correlate the planet mean density-orbital distance distribution with predictions from planet formation theories,- constrain the influence of planet migration and scattering on the architecture of multiple systems, and - specify how planet and system parameters change with host star characteristics, such as type, metallicity and age. The catalogue will allow us to study planets and planetary systems at different evolutionary phases. It will further provide a census for small, low-mass planets. This will serve to identify objects which retained their primordial hydrogen atmosphere and in general the typical characteristics of planets in such low-mass, low-density range. Planets detected by PLATO 2.0 will orbit bright stars and many of them will be targets for future atmosphere spectroscopy exploring their atmosphere. Furthermore, the mission has the potential to detect exomoons, planetary rings, binary and Trojan planets. The planetary science possible with PLATO 2.0 is complemented by its impact on stellar and galactic science via asteroseismology as well as light curves of all kinds of variable stars, together with observations of stellar clusters of different ages. This will allow us to improve stellar models and study stellar activity. A large number of well-known ages from red giant stars will probe the structure and evolution of our Galaxy. Asteroseismic ages of bright stars for different phases of stellar evolution allow calibrating stellar age-rotation relationships. Together with the results of ESA's Gaia mission, the results of PLATO 2.0 will provide a huge legacy to planetary, stellar and galactic science

Aplicabilidade da classificação de alcoolismo tipo A/tipo B Aplicability of the type A/type B classification of alcoholics

OBJETIVOS: Avaliar a aplicabilidade da tipologia e caracterizar os subtipos identificados. MÉTODOS: Características de 300 homens alcoolistas atendidos em um programa ambulatorial foram submetidas à análise de cluster para separá-los em dois subgrupos de acordo com a tipologia de Babor et al. Efetivaram-se cruzamentos de dados (significância avaliada pelo Teste do qui-quadrado de Pearson) para se verificar a associação dos clusters com variáveis clínicas e demográficas. RESULTADOS: Comparado ao outro grupo e pacientes, um dos clusters identificados foi caracterizado por um perfil de maior gravidade clínica. Pacientes do subtipo menos grave foram mais frequentemente (65,3%) encaminhados a tratamentos simbólicos, enquanto pacientes do subtipo mais grave foram atendidos predominantemente (58,5%) por abordagem exclusivamente farmacológica e aderiram mais ao tratamento proposto. CONCLUSÕES: Como os resultados identificaram subtipos de alcoolistas com distintas características, este estudo evidenciou a aplicabilidade clínica da tipologia de Babor et al. em nosso meio sociocultural¹. Também aponta para a relevância de estudos tipológicos que possam contribuir para uma mais ampla compreensão dos aspectos etiológicos, preventivos e terapêuticos do alcoolismo.<br>OBJECTIVE: To test the applicability of this typology and to characterize the identified subtypes. METHODS: Characteristics of 300 alcoholic men attending an out-treatment program were submitted to cluster analysis for identification of two subgroups (clusters), according to the original classification. Cross-tabulations were then performed to test for possible association of identified clusters to demographic and clinical features. Statistical significance was given by Pearson chi-square tests. RESULTS: Compared to the other group, one of the identified clusters was characterized by a more severe clinical profile. Patients of the mild subtype were principally (65,3%) referred to symbolic treatments while patients of the severe subtype were mainly assisted (58,5%) exclusively through a pharmacological approach and remained in treatment for longer periods of time. CONCLUSIONS: As the results identified subtypes of alcoholics with differential features, this study brought forth the clinical applicability of Babor et al. typology in our social-cultural context¹. Results also point to the relevance of typological studies that may contribute to a more adequate understanding of etiological, preventive and therapeutic aspects of alcoholism

Positive effects of a cognitive-behavioral intervention program for family caregivers of demented elderly

OBJECTIVE: It was to examine the effects of a Cognitive-Behavioral Therapy (CBT) program administered to family caregivers of dementia patients. METHODS: Forty family caregivers were enrolled in a CBT intervention across eight weekly sessions. Cognitive, functional and behavioral status of patients were evaluated, as well as their own and their family caregivers' perceptions of quality of life. Specific instruments were also applied to evaluate caregiver stress level, coping, anxiety and depression. RESULTS: At the end of the program, family caregivers reported fewer neuropsychiatric symptoms among patients and an improvement in patients' quality of life. In addition, caregivers changed their coping strategies, whereas a significant decrease was observed in their anxiety levels. CONCLUSION: The CBT program employed appears to be a promising and useful tool for clinical practice, displaying positive effects on quality of life and neuropsychiatric symptoms of dementia, as well as proving beneficial for alleviating anxiety and stress in family caregivers