908 resultados para 14 alpha-dihydroxy-13(15)-ene-16(12 alpha)-abietanolide
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Crop and livestock summaries for the state of Iowa, produced by the Iowa Department of Agriculture. Previously Agri-News
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Al ser un deporte relativamente nuevo, tiene 60 a?os de historia, no se cuenta con la suficiente bibliograf?a para su ense?anza, y mucho menos en las categor?as juveniles, es por eso que se quiere brindar un documento que, a partir de la experiencia en el campo y tomando modelos pedag?gicos de diferentes ?reas que no s?lo incluyen la educaci?n f?sica, con el cual los profesores de educaci?n f?sica y deporte puedan iniciar procesos formativos en menores de 16 a?os. Para llevar a cabo lo anterior, se pretende abordar temas que van m?s all? del entrenamiento deportivo juvenil, con el fin de brindar herramientas que permitan consolidar un grupo de trabajo cooperativo que abarque, desde la convocatoria de los ni?os, el trato y la participaci?n de los padres de familia, la organizaci?n de las sesiones de entrenamiento, hasta la conducci?n de procesos de autorregulaci?n, que incluyen el dialogo y el respeto como herramientas para la soluci?n de conflictos dentro y fuera del entrenamiento. Por lo tanto el presente trabajo de investigaci?n se estructur? en tres cap?tulos fundamentales que son: Capitulo uno hace referencia al planteamiento dial?ctico y epistemol?gico de la investigaci?n en donde se puede apreciar una correcta relaci?n entre el problema y los objetivos. En el cap?tulo dos encontramos una gran variedad de estudios internacionales y nacionales que nos permiten definir las tendencias m?s importantes del ult?mate y a partir de all? se realiza un an?lisis de c?mo han evolucionado en los ?ltimos tiempos el proceso de ense?anza- aprendizaje. Y en el tercer cap?tulo presentamos fase a fase el dise?o y elaboraci?n de la metodolog?a que proponemos para guiar el proceso de ense?anza ? aprendizaje en la muestra objeto de estudio, para finalmente realizar un an?lisis y discusi?n de resultados.
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Two IS- and 16-residue peptides containing a-aminoisobutyric acid (Aib) have been synthesized, as part of a strategy to construct stereochemically rigid peptide helices, in a modular approach to design of protein mimics. The peptides Boc-(Val-Ala-Leu-Aib),-OMe ( I ) and Boc-Val-Ala-Leu-Aib-Val-Ala-Leu-(Val-Ala-Leu-Aib()11z)- OhaMvee been crystallized.Both crystals are stable only in the presence of mother liquor or water. The crystal data are as follows. I: C78H140N16019~2H20,P2,, a = 16.391 (3) A, b = 16.860 (3) A, c = 18.428 (3) A, p = 103.02 (I)O, Z = 2, R = 9.6% for 3445 data with lFol >30(F), resolution 0.93 A. 11: C7,Hl,,N,S018.7.5H,0, C2221, a = 18.348 ( 5 ) A, b = 47.382 (1 1) A, c = 24.157 ( 5 ) A, Z =8, R = l0,6%, for 3147 data with lFol > 3a(F), resolution 1.00 A. The 15-residue peptide (11) is entirely a helical, while the 16-residue peptide ( I ) has a short segment of 310 helix at the N terminus. The packing of the helices in the crystals is rather incfficicnt with no particular attractions between Leu-Leu side chains, or any other pair. Both crystals have fairly large voids, which are filled with water molecules in a disordered fashion. Water molecule sites near the polar head-to-tail regions are well detcrmined, those closer to the hydrophobic side chains less so and a number of possible water sites in the remaining "empty" space are not determined. No interdigitation of Leu side chains is observed in the crystal as is hypothesized in the "leucine zipper" class of DNA binding proteins.
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Described in this thesis are measurements made of the thick-target neutron yield from the reaction 13C(α, n)16O. The yield was determined for laboratory bombarding energies between 0.475 and 0.700 MeV, using a stilbene crystal neutron detector and pulse-shape discrimination to eliminate gamma rays. Stellar temperatures between 2.5 and 4.5 x 108 oK are involved in this energy region. From the neutron yield was extracted the astrophysical cross-section factor S(E), which was found to fit a linear function: S(E) = [(5.48 ± 1.77) + (12.05 ± 3.91)E] x 105 MeV-barns, center-of-mass system. The stellar rate of the 13C(α, n)16O reaction if calculated, and discussed with reference to helium burning and neutron production in the core of a giant star.
Results are also presented of measurements carried out on the reaction 9Be(α, n)12C, taken with a thin Be target. The bombarding energy-range covered was from 0.340 to 0.680 MeV, with excitation curves for the ground- and first excited-state neutrons being reported. Some angular distributions were also measured. Resonances were found at bombarding energies of ELAB = 0.520 MeV (ECM = 0.360 MeV, Γ ~ 55 keV CM, ωγ = 3.79 eV CM) and ELAB = 0.600 MeV (ECM = 0.415 MeV, Γ ˂ 4 keV CM, ωγ = 0.88 eV CM). The astrophysical rate of the 9Be(α, n)12C reaction due to these resonances is calculated.
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The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)F-17 reaction has been studied by using the resonant scattering of F-17+p. The experiment was done at REX-ISOLDE CERN with the Miniball setup. The thick target method in inverse kinematics was utilized in the present experiment where a 44.2 MeV F-17 beam bombarded a similar to 40 mu m thick (CH2)(n) target. The inelastic scattering protons in coincidence with the de-excited 495 keV gamma rays have been clearly seen and they are from the inelastic branch to the first excited state in F-17 following decay of the 1(-) resonance in Ne-18. Some preliminary results are reported.
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The multistep syntheses of several bicyclic triamines are described, all of which have an imbedded 1,5,9-triazacyclododecane ring. In 1,5,9-triazabicyclo[7.3.3]pentadecanes 12, 13, 15, and 16, two nitrogens are bridged by three carbons. The monoprotonated forms of these triamines are highly stabilized by a hydrogen-bonded network involving the bridge and both bridgehead nitrogens, producing a difference of more than 8 pK(a) units in acidities of their monoprotonated and diprotonated forms. The one- and zero-carbon bridges in 1,5,9-triazabicyclo[9.1.1]tridecane (23) and 7-methyl-1,5,9-triazabicyclo[5.5.0]dodecane (39) do not enhance the stabilities of their monoprotonated forms. X-ray crystal structures and computational studies of 12.HI and 16.HI reveal similar, but somewhat weaker, hydrogen-bonded networks, relative to 15.HI. The activation free energies for conformational inversion of 13.HI (14.4 +/- 0.2 kcal/mol), 16.HI (15.0 +/- 0.1 kcal/mol) and 16 (8.8 +/- 0.3 kcal/mol) were measured by variable-temperature H-1 and C-13 NMR spectroscopy. These experimental barriers give an estimate of 6.2 kcal/mol for the strength of the bifurcated hydrogen bond between the bridge nitrogen and cavity proton in 16.HI. Computational studies support the hypothesis that N-inversion occurs in an open conformation, leading to an estimate of 10.32 kcal/mol for the enthalpy of the bifurcated hydrogen bond in 16.HI in the gas phase.
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Various authors have suggested that the gamma-ray burst (GRB) central engine is a rapidly rotating, strongly magnetized, (similar to 10(15)-10(16) G) compact object. The strong magnetic field can accelerate and collimate the relativistic flow and the rotation of the compact object can be the energy source of the GRB. The major problem in this scenario is the difficulty of finding an astrophysical mechanism for obtaining such intense fields. Whereas, in principle, a neutron star could maintain such strong fields, it is difficult to justify a scenario for their creation. If the compact object is a black hole, the problem is more difficult since, according to general relativity it has ""no hair"" (i.e., no magnetic field). Schuster, Blackett, Pauli, and others have suggested that a rotating neutral body can create a magnetic field by non-minimal gravitational-electromagnetic coupling (NMGEC). The Schuster-Blackett form of NMGEC was obtained from the Mikhail and Wanas`s tetrad theory of gravitation (MW). We call the general theory NMGEC-MW. We investigate here the possible origin of the intense magnetic fields similar to 10(15)-10(16) G in GRBs by NMGEC-MW. Whereas these fields are difficult to explain astrophysically, we find that they are easily explained by NMGEC-MW. It not only explains the origin of the similar to 10(15)-10(16) G fields when the compact object is a neutron star, but also when it is a black hole.
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Bioactivity-guided fractionation of several bioactive extracts obtained from Cerrado and Atlantic Forest plant species led to the isolation of potent DNA-damaging piperidine 1-5 and guanidine alkaloids 6-9 from Cassia leptophylla and Pterogyne nitens respectively, two common Leguminosae from Atlantic Forest. By means of biotechnological approach on Maytenus aquifolium, a species from Cerrado, moderate DNA-damaging sesquiterpene pyridine alkaloid 10-11 was isolated. Bioassay-guided fractionation on Casearia sylvestris, a medicinal plant species found in Cerrado and Atlantic Forest, led to the isolation of clerodane diterpenes 12-13 which showed effect on DNA. In addition, we have reported several interesting potent antifungal iridoids: 1β-hydroxy-dihydrocornin (14), 1α-hydroxy-dihydrocornin (15), α-gardiol (16), β-gardiol (17), plumericin (18), isoplumericin (19), 11-O-trans-caffeoylteucrein (20); ester derivative: 2-methyl-4-hydroxy-butyl-caffeoate (21), amide N-[7-(3'.4'-methylenedioxyphenyl)-2Z, 4Z-heptadienoyl] pyrrolidine (22) and triterpene viburgenin (23).
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Esta pesquisa analisa o desenvolvimento da espermatogênese em caititus (Tayassu tajacu) e determina a idade em que atingem a puberdade, considerando-se a biometria testicular e dos túbulos seminíferos, a quantificação das células espermatogênicas, a descrição morfológica dos estádios do ciclo do epitélio seminífero (CES), a freqüência relativa com a qual aparecem no interior dos túbulos seminíferos e o rendimento geral da espermatogênese. No experimento, os animais foram divididos de acordo com a faixa etária, em cinco grupos, com três animais em cada grupo, sendo G1 (7 a 8 meses), G2 (9 a 10 meses), G3 (11 a 12 meses), G4 (13 a 14 meses) e G5 (15 a 16 meses). Os animais foram submetidos à cirurgia de orquiectomia, para obtenção das amostras testiculares, as quais foram fixadas em solução de Alfac por 24 horas e processadas histologicamente, onde cortes de 5 μm foram corados em Hematoxilina-Eosina. Tendo como base, o método da morfologia tubular, foi feita a quantificação dos tipos celulares corrigidos para seus diâmetros nucleares médios de 10 secções transversais de túbulos seminíferos no estádio 1 do CES para animais com a espermatogênese estabelecida e 20 secções transversais para os animais mais jovens, nos quais não havia atividade espermatogênica estabelecida; e também a classificação dos estádios do ciclo do epitélio seminífero, por meio da análise de 100 secções transversais de túbulos seminíferos. Os dados da biometria testicular, a saber, o peso, o comprimento e a largura, revelaram crescimento constante e gradual com diferenças estatísticas significativas (p<0,05) e alta correlação entre si. Os valores do diâmetro tubular apresentaram significância estatística do G1 ao G4, a partir deste, tiveram crescimento acelerado e contínuo, não havendo significância estatística (p >0,05). De acordo com as análises quantitativas e morfológicas das células espermatogênicas que compõem o epitélio germinativo, os grupos etários dos animais foram classificados nas fases seguintes: impúbere (G1), pré-púbere (G2), puberdade (G3), pós-puberdade 1 (G4) e pós-puberdade 2 (G5). A fase em que ocorreu o início da atividade reprodutiva, ou seja, a puberdade, foi determinada nos animais a partir de 11 meses de idade, onde ocorreu o maior crescimento no número de células espermatogênicas e uma correlação positiva com o peso testicular. Nessa fase, as células de Sertoli, apresentaram um decréscimo significativo (p<0,05). Na determinação da freqüência relativa dos estádios do ciclo do epitélio seminífero, foram observadas oito tipos de associações, segundo o método da morfologia tubular, onde o estádio com maior e menor freqüências foram o 1 e o 3, respectivamente. A fase pós-meiótica, apresentou maior freqüência e a fase meiótica, a menor, sendo estatisticamente significativa em relação às demais. A eficiência reprodutiva foi demonstrada por meio dos valores traduzidos pelas razões celulares entre as espermatogônias do tipo A e espermátides arredondadas, não tendo sido observado aumento significativo das espermátides arredondadas entre os grupos G3 ao G5 (p>0,05); e o índice das células de Sertoli apresentou diferença estatística significativa entre todas as possíveis comparações dos grupos etários do G3 ao G5 (p <0,05).