The timing of synaptic vesicle endocytosis.

Alternative models to describe the endocytosis phase of synaptic vesicle recycling are associated with time scales of vesicle recovery ranging from milliseconds to tens of seconds. There have been suggestions that one of the major models, envisioned as a slow process that occurs only after complete fusion of the vesicle membrane with the neurolemma, might be applicable only under conditions of heavy, nonphysiological stimulation. Using FM 1-43 and similar fluorescent probes to label recycling synaptic vesicles in rat hippocampal neurons, we have measured the kinetics of endocytosis with a wide range of action-potential-driven exocytotic loads. Our results indicate that when either 5% or 25% of the vesicle pool is used, vesicles are recovered with a half-time on the order of 20 s (24 degrees C). This endocytosis rate was not influenced by operations designed to alter intracellular Ca2+ during membrane retrieval, suggesting that residual Ca2+ after strong stimuli probably does not greatly retard endocytosis. Finally, we have shown that vesicle-destaining kinetics are not strongly influenced by the substantially differing rates at which two marker dyes tested dissociate from membranes. This observation suggests that vesicles remain open long enough for essentially complete dissociation of even the slower dye (a few seconds) or, alternatively, that both dyes readily escape vesicle membrane by lateral diffusion through any exocytotic opening. These data seem most consistent with applicability of the slow-endocytosis, complete-fusion model at low as well as high levels of exocytosis.

Crossover and noncrossover recombination during meiosis: timing and pathway relationships.

During meiosis, crossovers occur at a high level, but the level of noncrossover recombinants is even higher. The biological rationale for the existence of the latter events is not known. It has been suggested that a noncrossover-specific pathway exists specifically to mediate chromosome pairing. Using a physical assay that monitors both crossovers and noncrossovers in cultures of yeast undergoing synchronous meiosis, we find that both types of products appear at essentially the same time, after chromosomes are fully synapsed at pachytene. We have also analyzed a situation in which commitment to meiotic recombination and formation of the synaptonemal complex are coordinately suppressed (mer1 versus mer1 MER2++). We find that suppression is due primarily to restoration of meiosis-specific double-strand breaks, a characteristic of the major meiotic recombination pathway. Taken together, the observations presented suggest that there probably is no noncrossover-specific pathway and that restoration of intermediate events in a single pairing/recombination pathway promotes synaptonemal complex formation. The biological significant of noncrossover recombination remains to be determined, however.

Fast-timing study of the l-forbidden 1/2(+) -> 3/2(+) M1 transition in Sn-129

The levels in Sn-129 populated from the beta(-) decay of In-129 isomers were investigated at the ISOLDE facility of CERN using the newly commissioned ISOLDE Decay Station (IDS). The lowest 1/2(+) state and the 3/2(+) ground state in 129Sn are expected to have configurations dominated by the neutron s(1/2) (l = 0) and d(3/2) (l = 2) single-particle states, respectively. Consequently, these states should be connected by a somewhat slow l-forbidden M1 transition. Using fast-timing spectroscopy we havemeasured the half-life of the 1/2(+) 315.3-keV state, T-1/2 = 19(10) ps, which corresponds to a moderately fast M1 transition. Shell-model calculations using the CD-Bonn effective interaction, with standard effective charges and g factors, predict a 4-ns half-life for this level. We can reconcile the shell-model calculations to the measured T-1/2 value by the renormalization of the M1 effective operator for neutron holes.

Estudo da qualidade do mel de abelhas sem ferrão por análise por ativação neutrônica instrumental

O Brasil é um dos maiores produtores mundiais de mel, no qual sua produção é baseada principalmente na criação da espécie exótica Apis mellifera. A produção de mel da Apis mellifera é cerca de 10 vezes maior que das espécies de abelhas sem ferrão, contudo, o mel de abelhas nativas possui maior valor comercial. Embora pouco explorado, o mel de abelhas sem ferrão desperta interesse em indústrias de cosméticos e medicinas naturais. A sua produção se apresenta como uma ferramenta com grande potencial para agregar valor econômico aos ecossistemas brasileiros, em especial os florestais, de forma sustentável e com menor potencial de influências de contaminantes traços. A qualidade química do mel é um importante requisito comercial, principalmente o destinado à exportação. Como exemplo, a União Européia em 2006 decidiu suspender a importação do mel produzido no Brasil sob alegação de que o país não possuía equivalência ao bloco quanto as diretrizes para o controle de resíduos e qualidade do produto. Diante do potencial de produção comercial sustentável do mel de abelhas nativas brasileiras e a falta de conhecimento sobre possíveis resíduos encontrados em sua composição, em especial os elementos traços, como objetivo principal deste trabalho pretendeu-se caracterizar a composição de elementos químicos do mel de abelhas sem ferrão, comparar com o de Apis mellifera e verificar as possíveis variações causadas pelo ambiente. Este estudo investigou a composição química dos méis de abelhas sem ferrão de cinco estados brasileiros: Bahia, Minas Gerais, Rio Grande do Norte, Santa Catarina e São Paulo; compreendendo um total de 70 colméias de diferentes espécies: Melipona quadrifasciata, Melipona scutelaris, Melipona mandacaia, Melipona capixaba, Melipona rufiventris, Melipona compressipes, Melipona bicolor, Nannotrigona testaceicornis, Tetragona clavipes, Tetragonisca angustula e Scaptotrigona sp.. Pólen, a principal fonte de minerais para a colméia, e as próprias abelhas foram também coletadas para estudos de composição e correlação com os méis. A análise por ativação neutrônica instrumental permitiu a determinação de Br, Ca, Co, Cs, Fe, La, Na, Rb, Sc e Zn nos méis, Br, Ca, Co, Cs, Fe, K, La, Na, Rb, Sc, Se e Zn nas amostras de pólen e As, Br, Co, Cr, Cs, Fe, K, La, Na, Rb, Sb, Sc, Se e Zn em abelhas. Méis das abelhas da subtribo trigonina apresentaram maiores concentrações dos elementos alcalinos. Alta razão K/Na foram observadas nas amostras de mel e pólen. Pólen se apresentou como uma grande fonte de P e Se. Análises quimiométricas indicaram os méis e abelhas como bons indicadores de atividades antrópicas. Arsênio apareceu nas abelhas coletadas em áreas de maior atividade antrópica. Como resultado, este estudo tem demonstrado o potencial nutracêutico do mel e pólen meliponícola e o potencial das abelhas nativas como ferramentas de avaliação da qualidade ambiental. A proximidade a atividades antrópicas mostrou-se fator decisivo para concentrações mais elevadas de As mas abelhas

Pulsar timing irregularities and the imprint of magnetic field evolution

Context. The rotational evolution of isolated neutron stars is dominated by the magnetic field anchored to the solid crust of the star. Assuming that the core field evolves on much longer timescales, the crustal field evolves mainly though Ohmic dissipation and the Hall drift, and it may be subject to relatively rapid changes with remarkable effects on the observed timing properties. Aims. We investigate whether changes of the magnetic field structure and strength during the star evolution may have observable consequences in the braking index n. This is the most sensitive quantity to reflect small variations of the timing properties that are caused by magnetic field rearrangements. Methods. We performed axisymmetric, long-term simulations of the magneto-thermal evolution of neutron stars with state-of-the-art microphysical inputs to calculate the evolution of the braking index. Relatively rapid magnetic field modifications can be expected only in the crust of neutron stars, where we focus our study. Results. We find that the effect of the magnetic field evolution on the braking index can be divided into three qualitatively different stages depending on the age and the internal temperature: a first stage that may be different for standard pulsars (with n ~ 3) or low field neutron stars that accreted fallback matter during the supernova explosion (systematically n < 3); in a second stage, the evolution is governed by almost pure Ohmic field decay, and a braking index n > 3 is expected; in the third stage, at late times, when the interior temperature has dropped to very low values, Hall oscillatory modes in the neutron star crust result in braking indices of a high absolute value and both positive and negative signs. Conclusions. Current magneto-thermal evolution models predict a large contribution to the timing noise and, in particular, to the braking index, from temporal variations of the magnetic field. Models with strong (≳ 1014 G) multipolar or toroidal components, even with a weak (~1012 G) dipolar field are consistent with the observed trend of the timing properties.

Fast X-ray transients towards the Galactic bulge with the Rossi X-ray Timing Explorer

In X-ray binaries, rapid variability in X-ray flux of greater than an order of magnitude on time-scales of a day or less appears to be a signature of wind accretion from a supergiant companion. When the variability takes the form of rare, brief, bright outbursts with only faint emission between them, the systems are called supergiant fast X-ray transients (SFXTs). We present data from twice-weekly scans of the Galactic bulge by the Rossi X-ray Timing Explorer that allow us to compare the behaviour of known SFXTs and possible SFXT candidates with the persistently bright supergiant X-ray binary 4U 1700−377. We independently confirm the orbital periods reported by other groups for SFXTs SAX J1818.6−1703 and IGR J17544−2619. The new data do not independently reproduce the orbital period reported for XTE J1739−302, but slightly improve the significance of the original result when the data are combined. The bulge source XTE J1743−363 shows a combination of fast variability and a long-term decline in activity, the latter behaviour not being characteristic of supergiant X-ray binaries. A far-red spectrum of the companion suggests that it is a symbiotic neutron star binary rather than a high-mass binary, and the reddest known of this class: the spectral type is approximately M8 III.

Pulse phase-coherent timing and spectroscopy of CXOU J164710.2−45521 outbursts

We present a long-term phase-coherent timing analysis and pulse-phase resolved spectroscopy for the two outbursts observed from the transient anomalous X-ray pulsar CXOU J164710.2−455216. For the first outburst we used 11 Chandra and XMM–Newton observations between 2006 September and 2009 August, the longest baseline yet for this source. We obtain a coherent timing solution with P = 10.61065583(4) s, Ṗ = 9.72(1) × 10−13 s s−1 and P̈ = –1.05(5) × 10−20 s s−2. Under the standard assumptions this implies a surface dipolar magnetic field of ∼1014 G, confirming this source as a standard B magnetar. We also study the evolution of the pulse profile (shape, intensity and pulsed fraction) as a function of time and energy. Using the phase-coherent timing solution we perform a phase-resolved spectroscopy analysis, following the spectral evolution of pulse-phase features, which hints at the physical processes taking place on the star. The results are discussed from the perspective of magnetothermal evolution models and the untwisting magnetosphere model. Finally, we present similar analysis for the second, less intense, 2011 outburst. For the timing analysis we used Swift data together with 2 XMM–Newton and Chandra pointings. The results inferred for both outbursts are compared and briefly discussed in a more general framework.

The Contents and Timing of a European Banking Union: Reflections on the differing views. CEPS Essay (No. 2), 30 November 2012

Although views differ on the precise contents and timing of a genuine banking union, there is wide political agreement in principle on the need for three basic and vital elements: European bank supervision, a European deposit guarantee scheme (DGS) and a European bank resolution mechanism. In this CEPS Essay, H. Onno Ruding offers his personal views on the progress achieved to date, the outstanding issues that will prove the most difficult to resolve and recommendations on the way forward.

Germany and the Eurocrisis: The timing of politics and the politics of timing. ACES Cases No. 2014.3

This paper speculates on the future of the euro. It uses Germany as a prism for the discussion about what might be done next to bolster the Euro. Researching the future—always a challenging task—is made harder when multiple state actors contend for prominence on the basis of shifting coalitions at home, all while interacting at an international level. That said, almost everyone accepts that German choices will play the central role in the path ultimately chosen. This paper thus foregrounds Germany’s role in shaping the way ahead, and it does so through an explicitly political framework focused primarily on the electoral implausibility of an alternative German policy course.

The Interregional Association Agreement between the European Union and Mercosur: Is the Timing Right? Bruges Political Research Papers 46/2015.

The European Union (EU) and Mercosur talks have been stalled since discussions were resumed in 2000. Recurring protectionist and institutional obstacles have slowed down negotiations. The financial crisis, however, has resulted in low domestic demand in the EU. This has made the interregional association agreement (IAA) with Mercosur more attractive. The loss of the Generalized Scheme of Preference (GSP) status and the lack of a Free Trade Agreement (FTA) with the EU have both disadvantaged Mercosur. A further window of opportunity is opening up in Mercosur. In Brazil, there have been cries for a change in government. In Argentina, presidential elections will take place in October 2015 and will assuredly bring an end to Kirchnerismo. A change in leadership in both countries is expected to make agreement more likely. Protectionist policies are not expected to remain as high if there is change in government. This will provide the EU with an opportunity to advance the negotiations and conclude the IAA.

Sistema de gestão de energia e ativação de uma espoleta eletrónica

Os incêndios florestais constituem uma realidade que pode ser minimizada com o auxílio Forças Armadas, através de homens e de meios. O Projeto FIREND®, no qual este trabalho está inserido, tem como objetivo projetar uma munição que ao libertar uma substância química sobre o fogo, o impeça de se expandir e se possível, o extinga. O projétil tem 155mm de calibre e o seu compartimento de carga terá cerca de 7,5

Democratic planning in action; time for timing.

Mode of access: Internet.

Prevalence and timing of oral sex with opposite-sex partners among females and males aged 15-24 years : United States, 2007-2010 /

Mode of access: Internet.