Direct Detection of YORP Spin-up on Asteroid (25143) Itokawa and Implications for its Internal Structure

Near-Earth asteroid (25143) Itokawa was visited by the Hayabusa spacecraft in 2005, resulting in a highly detailed surface shape and topography model. This model has led to several predictions for the expected radiative torques on this asteroid, suggesting that its spin rate should be decelerating. Through an observational survey spanning 2001 to 2013 we have successfully measured an acceleration in its spin rate of dω/dt = 3.54 (± 0.38) × 10^(-8) rad day^(-2), equivalent to a decrease of its rotation period of ~ 45 ms year^(-1). Using the shape model determined from the Hayabusa spacecraft, we applied a detailed thermophysical analysis, to reconcile the predicted YORP strength with that observed. We find that the center-of-mass for Itokawa must be shifted by ~20 m along the long-axis of the asteroid to reconcile observations with theory. This can be explained if Itokawa is composed of two separate bodies with very different bulk densities of 1740 ± 110 kg m^(-3) and 2730 ± 440 kg m^(-3), and was formed from the merger of two separate bodies, consistent with the collapse of a binary system or the re-accumulation of material from a catastrophic collisional disruption. We demonstrate that an observational measurement of radiative torques, when combined with a detailed shape model, can provide insight into the interior structure of an asteroid.

Thermal properties and eutectic behaviour of dapivirine in combination with steroid hormones and other antiretrovirals

Background: Combination drug products can display thermal behaviour that is more complex than for the corresponding single drug products. For example, the contraceptive vaginal ring (VR) Nuvaring contains a eutectic (lowest melting) composition of etonogestrel (ETN) and ethinyl estradiol. Here we report the predisposition of dapivirine (DPV) to form reduced melting/eutectic mixtures when combined with other contraceptive hormones and antiretrovirals, and discuss the implications for development of combination microbicide and multipurpose prevention technology (MPT) products.
Methods: Binary mixtures of DPV with darunavir (DRV), levonorgestrel (LNG), ETN or maraviroc (MVC) were prepared either by physical mixing or by solvent evaporation. Selected binary mixtures were also incorporated into silicone elastomer (SE) VR devices. Thermal behavior of the mixtures was analyzed using differential scanning calorimetry (DSC) operating in standard heating ramp mode (10 °C/min). DSC data were used to construct two component phase diagrams for each binary system.
Results: Drug mixtures typically showed reduced melting transitions for both drug components, with clear evidence for a eutectic mixture at a well-defined intermediate composition. Eutectic temperatures and compositions for the various mixtures were: 40% DPV / 60% ETN - 170°C; 25% DPV / 75% MVC - 172°C; 65% DPV / 35% LNG - 192°C. In each case, the eutectic composition was also detected when the drug mixtures were incorporated into SE VRs. For the DPV/DRV system, the thermal behaviour is complicated by desolvation from the darunavir ethanolate polymorph.
Conclusions: When DPV is combined with small molecular weight hydrophobic drugs, the melting temperature for both drugs is typically reduced to a degree dependent on the composition of the mixture. At specified compositions, a low melting eutectic system results. The formation of eutectic behavior in binary drug systems needs to be carefully characterised in order to define product performance and drug release.

Solid–liquid equilibria in systems [Cxmim][Tf2N] with diethylamine

In the present work, the solid–liquid–liquid equilibrium in the binary system of diethylamine (1) and ionic liquid (2) 1-methyl-3-ethylimidazolium bis(trifluoromethylsulfonyl)imide and solid–liquid equilibrium in system 1-methyl-3-butylimidazolium bis(trifluoromethylsulfonyl)imide was studied. Phase equilibrium was determined experimentally by means of a polythermic method. These data were then used to determine the activity coefficients for both ionic liquids. For the pure diethylamine the enthalpy of fusion was determined by differential scanning calorimetry, because to the best of our knowledge, this data is not yet reported in the open literature, a contrario of pure ionic liquids tested during this work.

Deflagrations in hybrid CONe white dwarfs: a route to explain the faint Type Iax supernova 2008ha

Stellar evolution models predict the existence of hybrid white dwarfs (WDs) with a carbon-oxygen core surrounded by an oxygen-neon mantle. Being born with masses similar to 1.1 M-aS (TM), hybrid WDs in a binary system may easily approach the Chandrasekhar mass (M-Ch) by accretion and give rise to a thermonuclear explosion. Here, we investigate an off-centre deflagration in a near-M-Ch hybrid WD under the assumption that nuclear burning only occurs in carbon-rich material. Performing hydrodynamics simulations of the explosion and detailed nucleosynthesis post-processing calculations, we find that only 0.014 M-aS (TM) of material is ejected while the remainder of the mass stays bound. The ejecta consist predominantly of iron-group elements, O, C, Si and S. We also calculate synthetic observables for our model and find reasonable agreement with the faint Type Iax SN 2008ha. This shows for the first time that deflagrations in near-M-Ch WDs can in principle explain the observed diversity of Type Iax supernovae. Leaving behind a near-M-Ch bound remnant opens the possibility for recurrent explosions or a subsequent accretion-induced collapse in faint Type Iax SNe, if further accretion episodes occur. From binary population synthesis calculations, we find the rate of hybrid WDs approaching M-Ch to be of the order of 1 per cent of the Galactic SN Ia rate.

Total eclipse of the heart: the AM CVn Gaia14aae/ASSASN-14cn

We report the discovery and characterization of a deeply eclipsing AM CVn-system, Gaia14aae (=ASSASN-14cn). Gaia14aae was identified independently by the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al.) and by the Gaia Science Alerts project, during two separate outbursts. A third outburst is seen in archival Pan-STARRS-1 (PS1; Schlafly et al.; Tonry et al.; Magnier et al.) and ASAS-SN data. Spectroscopy reveals a hot, hydrogen-deficient spectrum with clear double-peaked emission lines, consistent with an accreting double-degenerate classification. We use follow-up photometry to constrain the orbital parameters of the system. We find an orbital period of 49.71 min, which places Gaia14aae at the long period extremum of the outbursting AM CVn period distribution. Gaia14aae is dominated by the light from its accreting white dwarf (WD). Assuming an orbital inclination of 90° for the binary system, the contact phases of the WD lead to lower limits of 0.78 and 0.015 M⊙ on the masses of the accretor and donor, respectively, and a lower limit on the mass ratio of 0.019. Gaia14aae is only the third eclipsing AM CVn star known, and the first in which the WD is totally eclipsed. Using a helium WD model, we estimate the accretor's effective temperature to be 12 900 ± 200 K. The three outburst events occurred within four months of each other, while no other outburst activity is seen in the previous 8 yr of Catalina Real-time Transient Survey (CRTS; Drake et al.), Pan-STARRS-1 and ASAS-SN data. This suggests that these events might be rebrightenings of the first outburst rather than individual events.

Probing The effects of Experimental Conditions on the Character of Drug-Polymer Phase Diagrams Constructed Using Flory-Huggins Theory

Purpose: Amorphous drug-polymer solid dispersions have been found to result in improved drug dissolution rates when compared to their crystalline counterparts. However, when the drug exists in the amorphous form it will possess a higher Gibb’s free energy than its associated crystalline state and can recrystallize. Drug-polymer phase diagrams constructed through the application of the Flory Huggins (F-H) theory contain a wealth of information regarding thermodynamic and kinetic stability of the amorphous drug-polymer system. This study was aimed to evaluate the effects of various experimental conditions on the solubility and miscibility detections of drug-polymer binary system. Methods: Felodipine (FD)-Polyvinylpyrrolidone (PVP) K15 (PVPK15) and FD-Polyvinylpyrrolidone/vinyl acetate (PVP/VA64) were the selected systems for this research. Physical mixtures with different drug loadings were mixed and ball milled. These samples were then processed using Differential Scanning Calorimetry (DSC) and measurements of melting point (Tend) and glass transition (Tg) were detected using heating rates of 0.5, 1.0 and 5.0°C/min. Results: The melting point depression data was then used to calculate the F-H interaction parameter (χ) and extrapolated to lower temperatures to complete the liquid–solid transition curves. The theoretical binodal and spinodal curves were also constructed which were used to identify regions within the phase diagram. The effects of polymer selection, DSC heating rate, time above parent polymer Tg and polymer molecular weight were investigated by identifying amorphous drug miscibility limits at pharmaceutically relevant temperatures. Conclusion: The potential implications of these findings when applied to a non-ambient processing method such as Hot Melt Extrusion (HME) are also discussed.

A actividade sintética de hMSCs em contacto com vidros bioativos

Os vidros bioativos constituem um material apropriado para o preenchimento de defeitos ósseos, como alternativa a enxertos autólogos, uma vez que, quando expostos a fluidos fisiológicos promovem a formação de uma ligação com o tecido ósseo sob a forma de uma camada de hidroxiapatite carbonatada. No presente trabalho caracterizaram-se vidros bioativos sem conteúdo alcalino, cuja composição incide no sistema binário de diópsido (CaMgSi2O6) e fosfato de tricálcio (3CaO·P2O5), em função da sua molhabilidade, carga superficial, perfil de degradação, carácter bioativo em fluido fisiológico simulado e do seu comportamento in vitro em contacto com células estaminais mesenquimais humanas (hMSCs). A medição do ângulo de contacto inicial de água sobre os vidros demonstrou o carácter hidrofílico dos vidros investigados. A determinação do potencial zeta mostrou que a carga superficial dos vidros é negativa, sendo mais negativa na composição Di-70. O estudo da biodegradação dos vidros, efetuado através da sua imersão em Tris-HCl, permitiu concluir que a perda de peso dos vidros foi reduzida. A caraterização in vitro em meio acelular foi efetuada através da imersão dos vidros numa solução de fluido fisiológico simulado (SBF) e verificou-se que estes possuem capacidade de formar uma camada de hidroxiapatite carbonatada à sua superfície após 7 dias, detetável por XRD, FTIR e SEM/EDS, sugerindo que este conjunto de vidros é potencialmente bioativo, e poderá estimular a proliferação e diferenciação celular. A resposta das hMSCs em cultura aos vidros bioativos foi avaliada em termos de atividade metabólica, morfologia, viabilidade, proliferação e diferenciação osteogénica e conclui-se que os biovidros Di-60 e Di-70 poderão constituir um suporte viável para a proliferação e diferenciação de hMSCs.

Étude spectroscopique du système WR145: une étoile Wolf-Rayet hybride WN/C dont le vent entre en collision avec le vent de son compagnon O

Mémoire numérisé par la Division de la gestion de documents et des archives de l'Université de Montréal

Développement de tensioactifs à base d’acides biliaires pegylés pour des applications pharmaceutiques

Les acides biliaires sont reconnus comme des tensioactifs d’origine biologique potentiellement applicables dans le domaine pharmaceutique. Leurs structures en font une plateforme idéale pour l’obtention de nouvelles architectures polymères. Des composés synthétisés par polymérisation anionique de dérivés d’oxirane comme l’oxyde d’éthylène, offre des dérivés amphiphiles pegylés démontrant des propriétés d’agrégation intéressantes en vue d’une amélioration de la biocompatibilité et de la capacité d’encapsulation médicamenteuse. Une large gamme d’acides biliaires pegylés (BA(EGn)x) a été préparée avec comme objectif premier leurs applications dans la formulation de principes actifs problématiques. Pour cela, une caractérisation rigoureuse du comportement de ces dérivés (modulation de la longueur (2 < n < 19) et du nombre de bras (2 < x < 4) de PEG) en solution a été réalisée. Dans le but d’améliorer la biodisponibilité de principes actifs lipophiles (cas de l’itraconazole), des nanoémulsions spontanées, composées de BA(EGn)x et d’acide oléique, ont été développées. L’évaluation in vitro, de la toxicité (cellulaire), et de la capacité de solubilisation des systèmes BA(EGn)x, ainsi que les paramètres pharmacocinétiques in vivo (chez le rat), suggèrent une livraison contrôlée par nos systèmes auto-assemblés lors de l’administration orale et intraveineuse. Aussi, la synthèse de copolymères en blocs en étoile à base d’acide cholique pegylés a été effectuée par polymérisation anionique par addition d’un second bloc au caractère hydrophobe de poly(éther d’allyle et de glycidyle) (CA(EGn-b-AGEm)4). Selon le ratio de blocs hydrophiles-hydrophobes CA(EGn-b-AGEm)4, des réponses thermiques en solution (LCST) ont été observées par un point de trouble (Cp) entre 8 oC et 37 oC. Un mécanisme de formation d’agrégats en plusieurs étapes est suggéré. La thiolation des allyles des PAGE permet une fonctionnalisation terminale à haute densité, comparable aux dendrimères. Les caractérisations physico-chimiques des CA(EGn-b-AGEm-NH2)4 et CA(EGn-b-AGEm-COOH)4 indiquent la formation de structures auto-assemblées en solution, sensibles à la température ou au pH. Cette fonctionnalisation élargie le domaine d’application des dérivés d’acides biliaires pegylés en étoile vers la transfection d’ADN, la livraison de siRNA thérapeutiques ou encore à une sélectivité de livraison médicamenteux (ex. sensibilité au pH, greffage ligands).

Recherche et caractérisation de systèmes binaires dont l'une des composantes est de faible masse

Nous présentons la découverte de quatorze nouveaux systèmes binaires ayant une séparation supérieure à 250 UA et dont au moins l'une des composantes est une naine M ou une naine L. Ces systèmes ont d'abord été identifiés en cherchant des objets ayant un mouvement propre commun autour d'étoiles connues possédant un mouvement propre élevé, grâce à une corrélation croisée de grands relevés du ciel dans l'infrarouge proche (2MASS, SDSS et SIMP). Un suivi astrométrique, afin de confirmer le mouvement propre commun, a été réalisé sur toutes les cibles avec la caméra SIMON et/ou la caméra CPAPIR à l'Observatoire du Mont-Mégatic (OMM) ou à l'Observatoire interaméricain du Cerro Tololo (CTIO). Un suivi spectroscopique a aussi été effectué sur la plupart des compagnons avec GMOS ou GNIRS à Gemini afin de déterminer leurs types spectraux. La probabilité que deux objets forment un système binaire par hasard a été évaluée afin de s'assurer que les couples candidats que nous présentons soient réellement liés.Un de nos nouveaux systèmes a un compagnon de masse sous-stellaire : 2M1259+1001 (L4.5). L'étude des systèmes que nous avons découverts pourra, entre autre, nous aider à mieux comprendre les mécanismes de formation des étoiles de très faible masse et des naines brunes.

Studies on a New Vulcanization Syste

Studies on the chemistry of vulcanization” play a central role in the efforts to achieve better product performance from natural and synthetic rubbers. They provide rubber technologists with an increasingly realistic picture of molecular framework of vulcanizates, from which relation between physical properties and chemical constitution may be deduced. Moreover, these studies are also aimed at the understanding of the vulcanization process, in sufficiently advanced chemical mechanistic terms, so that the effect of changes on vulcanizate structure can rationally be predicted.“ The study of accelerator activity ofthe binary system containing ATU with TMTD, and with MBTS in sulphur vulcanization of dry natural rubber using standard procedures for compounding and vulcanization is described in the third chapter. The study of the gum vulcanizates form part I of this chapter The behaviour of the experimental mixes were compared with those of the controls containing thiourea; diphenyl guanidine

Joint importance of multistate systems

Importance measures in reliability engineering are used to identify weak areas of a system and signify the roles of components in either causing or contributing to proper functioning of the system. Traditional importance measures for multistate systems mainly concern reliability importance of an individual component and seldom consider the utility performance of the systems. This paper extends the joint importance concepts of two components from the binary system case to the multistate system case. A joint structural importance and a joint reliability importance are defined on the basis of the performance utility of the system. The joint structural importance measures the relationship of two components when the reliabilities of components are not available. The joint reliability importance is inferred when the reliabilities of the components are given. The properties of the importance measures are also investigated. A case study for an offshore electrical power generation system is given.

Fireballs in AE Aquarii

AE Aqr is an unusual cataclysmic variable star exhibiting bizarre phenomena that can now be interpreted in the context of a magnetic propeller that throws gas out of the binary system.

Near-infrared integral field spectroscopy of the Homunculus nebula around eta Carinae using Gemini/CIRPASS

This work presents the first integral field spectroscopy of the Homunculus nebula around eta Carinae in the near-infrared spectral region (J band). We confirmed the presence of a hole on the polar region of each lobe, as indicated by previous near-IR long-slit spectra and mid-IR images. The holes can be described as a cylinder of height (i.e. the thickness of the lobe) and diameter of 6.5 and 6.0 x 10(16) cm, respectively. We also mapped the blue-shifted component of He I lambda 10830 seen towards the NW lobe. Contrary to previous works, we suggested that this blue-shifted component is not related to the Paddle but it is indeed in the equatorial disc. We confirmed the claim of N. Smith and showed that the spatial extent of the Little Homunculus matches remarkably well the radio continuum emission at 3 cm, indicating that the Little Homunculus can be regarded as a small H II region. Therefore, we used the optically thin 1.3 mm radio flux to derive a lower limit for the number of Lyman-continuum photons of the central source in eta Car. In the context of a binary system, and assuming that the ionizing flux comes entirely from the hot companion star, the lower limit for its spectral type and luminosity class ranges from O5.5 III to O7 I. Moreover, we showed that the radio peak at 1.7 arcsec NW from the central star is in the same line-of-sight of the `Sr-filament` but they are obviously spatially separated, while the blue-shifted component of He I lambda 10830 may be related to the radio peak and can be explained by the ultraviolet radiation from the companion star.

Modelling the line variations from the wind-wind shock emissions of WR 30a

The study of Wolf-Rayet stars plays an important role in evolutionary theories of massive stars. Among these objects, similar to 20 per cent are known to be in binary systems and can therefore be used for the mass determination of these stars. Most of these systems are not spatially resolved and spectral lines can be used to constrain the orbital parameters. However, part of the emission may originate in the interaction zone between the stellar winds, modifying the line profiles and thus challenging us to use different models to interpret them. In this work, we analysed the He II lambda 4686 angstrom + C IV lambda 4658 angstrom blended lines of WR 30a (WO4+O5) assuming that part of the emission originate in the wind-wind interaction zone. In fact, this line presents a quiescent base profile, attributed to the WO wind, and a superposed excess, which varies with the orbital phase along the 4.6-d period. Under these assumptions, we were able to fit the excess spectral line profile and central velocity for all phases, except for the longest wavelengths, where a spectral line with constant velocity seems to be present. The fit parameters provide the eccentricity and inclination of the binary orbit, from which it is possible to constrain the stellar masses.