Classificação citoistológica, imunoistoquímica, lesão de DNA, morfometria e índice de proliferação celular dos linfomas em cães

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Estudo do potencial de transformação maligna do líquen plano bucal: análise histológica, histoquímica e imunoistoquímica

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Avaliação da proliferação celular, índice apoptótico e da expressão do P53 nos linfomas caninos

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Genotoxicity evaluation of environmental pollutants using analysis of nucleolar alterations

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Contribution of AT-, GC-, and methylated cytidine-rich DNA to chromatin composition in Malpighian tubule cell nuclei of Panstrongylus megistus (Hemiptera, Reduviidae)

The Malpighian tubule cell nuclei of male Panstrongylus megistus, a vector of Chagas disease, contain one chromocenter, which is composed solely of the Y chromosome. Considering that different chromosomes contribute to the composition of chromocenters in different triatomini species, the aim of this study was to determine the contribution of AT-, GC-, and methylated cytidine-rich DNA in the chromocenter as well as in euchromatin of Malpighian tubule cell nuclei of P. megistus in comparison with published data for Triatoma infestans. Staining with 4',6-diamidino-2-phenylindole/actinomycin D and chromomycin A(3)/distamycin, immunodetection of 5-methylcytidine and AgNOR test were used. The results revealed AT-rich/GC-poor DNA in the male chromocenter, but equally distributed AT and GC DNA sequences in male and female euchromatin, like in T. infestans. Accumulation of argyrophilic proteins encircling the chromocenter did not always correlate with that of GC-rich DNA. Methylated DNA identified by immunodetection was found sparsely distributed in the euchromatin of both sexes and at some points around the chromocenter edge, but it could not be considered responsible for chromatin condensation in the chromocenter, like in T. infestans. However, unlike in T. infestans, no correlation between the chromocenter AT-rich DNA and nucleolus organizing region (NOR) DNA was found in P. megistus. (c) 2011 Elsevier GmbH. All rights reserved.

Histomorphometrical and proliferative aspects of placenta and uterus of the collared peccary (Tayassu tajacu)

The histomorphometric and proliferative characteristics of the collared peccary (Tayassu tajacu) placenta and uterus were analyzed. The material was examined by standard histological techniques and histochemistry (PAS, Perls and Alcian Blue pH 0.5 and 2.5%) and the cellular proliferation by AgNORs and flow cytometry. All the analyzed morphometric variables differed between pregnant and non-pregnant uteri in the luteal phase using the Dunnet test. Height and gland diameter of uterine glands increased linearly during pregnancy, with an intense positive PAS and Perls reaction in all stages. The cells with more than seven AgNORs per nuclei and the cells in the G2M cell cycle phase in the maternal tissue also increased after 70 days of pregnancy. The uteroplacental ridges had a linear increase in size with two distinct areas, base and top, with uterine epithelium and trophoblastic cells changing their morphology following the placental ridge development. Flow cytometry analysis showed the percentage of cells in each cell cycle phase with a quadratic behavior for stages G2/M in the maternal tissue, suggesting an increase in proliferative capacity of maternal tissue after 65 days of pregnancy. The same quadratic effect was observed in the G0/G1 phase in both maternal and fetal tissues. Cells in apoptosis showed cubic behavior in both tissues. The morphometric and cellular dynamic aspects observed in this study have not been previously described and they extend our knowledge of functions relating to maternal-fetal dynamics in this species.

Efeitos da oxigenoterapia hiperbárica em lesões actícas da veia cava e aorta infra-renal. Estudo experimental em ratos

Objetivos: Estudar o efeito da Oxigenoterapia Hiperbárica sobre as lesões causadas pela radiação ionizante na veia cava e aorta. Método: Foram utilizados 32 ratos adultos distribuídos aleatoriamente em 4 grupos: 3 no grupo controle; 10 no grupo oxigenoterapia hiperbárica (5 sessões e 3 ATA e após 3 dias, operados), 9 no grupo radioterapia (8 sessões de 5Gy, atingindo 54Gy, sendo operados após 7 dias), 10 no grupo radioterapia e oxigenoterapia hiperbárica (procedimento radioterapia, observação por 7 dias, submetidos a 5 sessões de oxigenoterapia hiperbárica e após 3 dias, são operados. Ressecamos a veia cava e aorta infrarenal para estudo morfológico (integridade endotelial, infiltrado inflamatório e integridade da vasa-vasorum), avaliação do ciclo celular pelo método do AgNOR e índice de apoptose nas distintas camadas dos vasos, através da Caspase-3 (imuno-histoquímica). Resultados: O grupo radioterapia – oxigenoterapia hiperbárica apresentou diminuição estatisticamente significativa das alterações morfológicas em vasa-vasorum, aumento da atividade celular na camada média e também diminuição do índice de apoptose nas camadas íntima e média da aorta infra-renal quando comparados ao grupo apenas submetidos à radiação ionizante. A lesões rádio induzidas na veia cava não apresentaram melhora significativa com a oxigenoterapia hiperbárica Conclusão: A oxigenoterapia hiperbárica é capaz de minimizar as lesões radio-induzidas em fase aguda em aorta.

EChO

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the presence of life. EChO—the Exoplanet Characterisation Observatory—is a mission concept specifically geared for this purpose. EChO will provide simultaneous, multi-wavelength spectroscopic observations on a stable platform that will allow very long exposures. The use of passive cooling, few moving parts and well established technology gives a low-risk and potentially long-lived mission. EChO will build on observations by Hubble, Spitzer and ground-based telescopes, which discovered the first molecules and atoms in exoplanetary atmospheres. However, EChO’s configuration and specifications are designed to study a number of systems in a consistent manner that will eliminate the ambiguities affecting prior observations. EChO will simultaneously observe a broad enough spectral region—from the visible to the mid-infrared—to constrain from one single spectrum the temperature structure of the atmosphere, the abundances of the major carbon and oxygen bearing species, the expected photochemically-produced species and magnetospheric signatures. The spectral range and resolution are tailored to separate bands belonging to up to 30 molecules and retrieve the composition and temperature structure of planetary atmospheres. The target list for EChO includes planets ranging from Jupiter-sized with equilibrium temperatures T eq up to 2,000 K, to those of a few Earth masses, with T eq \u223c 300 K. The list will include planets with no Solar System analog, such as the recently discovered planets GJ1214b, whose density lies between that of terrestrial and gaseous planets, or the rocky-iron planet 55 Cnc e, with day-side temperature close to 3,000 K. As the number of detected exoplanets is growing rapidly each year, and the mass and radius of those detected steadily decreases, the target list will be constantly adjusted to include the most interesting systems. We have baselined a dispersive spectrograph design covering continuously the 0.4–16 μm spectral range in 6 channels (1 in the visible, 5 in the InfraRed), which allows the spectral resolution to be adapted from several tens to several hundreds, depending on the target brightness. The instrument will be mounted behind a 1.5 m class telescope, passively cooled to 50 K, with the instrument structure and optics passively cooled to \u223c45 K. EChO will be placed in a grand halo orbit around L2. This orbit, in combination with an optimised thermal shield design, provides a highly stable thermal environment and a high degree of visibility of the sky to observe repeatedly several tens of targets over the year. Both the baseline and alternative designs have been evaluated and no critical items with Technology Readiness Level (TRL) less than 4–5 have been identified. We have also undertaken a first-order cost and development plan analysis and find that EChO is easily compatible with the ESA M-class mission framework.

The romances of Alexandre Dumas ...

Illustrated by Edmund H. Garnett, J. Wagrez, E. Grivaz and others.

Cours d'agriculture,

Mode of access: Internet.

The schools of doubt and the school of faith /

Tr. of: Les écoles du doute et l'école de la foi.