Diante da escassez de estudos que correlacionem a remoção do disco ou da cartilagem articular do côndilo, sobretudo, na análise de parâmetros morfométricos, o presente estudo objetivou analisar, por meio de microtomografia, alterações da estrutura e qualidade óssea em ratos (Rattus norvegicus, albinos, Wistar). Os espécimes foram divididos em três grupos experimentais e a cirurgia ocorreu, em todos os grupos, do lado direito. No grupo experimental (RDC), deu-se a remoção do disco articular e remoção da cartilagem articular do lado direito; no grupo experimental (RD), somente remoção do disco articular do lado direito; no grupo experimental (SHAM), apenas acesso cirúrgico e posterior sutura sem danos ao disco articular ou cartilagem. Os côndilos foram analisados por microtomografia e executou-se comparação entre os lados de cada grupo e entre os grupos do lado direito e esquerdo. Os parâmetros morfométricos apontaram para um declínio da estrutura e qualidade óssea, sucessivamente, em ordem crescente, no lado operado dos grupos SHAM, RD e RDC. / Considering that only few studies on the correlation between temporomandibular joint (TMJ) disk removal and conditions of the cartilage of the condyle, especially in the analysis of morphometric parameters, this study aimed to analyze changes in the bone structure and quality in rats (Rattus norvegicus, albino Wistar) with micro-computed tomography. The specimens were divided into three groups that underwent surgery in the right TMJ. In the first experimental group, surgical procedures included both disk and joint cartilage removal (DCR). In the second experimental group, only the disk was removed during surgeries (DR), whereas in the control group (SHAM) only surgical access and subsequent suture without damaging the disc or joint cartilage was performed. The condyles were analyzed by micro-computed tomography and inter-group and intra-group side (left and right) comparisons were carried out. The morphometric parameters indicated a decline in bone structure and quality successively in the groups in ascending order of TMJ surgical damage (control group, SHAM, and the two experimental groups, DR and DCR).

Os parâmetros acústicos subjetivos são critérios que definem a qualidade acústica de uma sala de música. A apreciação musical dentro da sala é afetada por diversas impressões acústicas que ocorrem ao mesmo tempo. Cada uma dessas impressões é associada a um parâmetro acústico de natureza subjetiva que está correlacionado a uma grandeza física mensurável, constituindo um conjunto de parâmetros acústicos objetivos que formam uma base científica para a análise acústica das salas de música. Neste trabalho desenvolvemos pesquisa de âmbito teórico e experimental envolvendo a análise dos parâmetros acústicos subjetivos mais relevantes para a avaliação da qualidade acústica de salas de escuta musical. Fizemos um levantamento abrangente do material já publicado sobre o assunto, o que nos orientou a respeito das medições acústicas pertinentes à referida análise e nos permitiu formalizar as devidas conclusões. Implementamos e aplicamos a tecnologia necessária para a obtenção dos parâmetros. Determinamos a metodologia experimental mais adequada e efetuamos medições em seis importantes salas de concerto, comparando os resultados. Fizemos uma análise crítica a respeito dos parâmetros acústicos obtidos e aprofundamos a compreensão sobre seus significados e suas utilidades. Por fim, fizemos uma análise subjetiva de júri correlacionando os parâmetros acústicos medidos às respectivas impressões acústicas sobre amostras musicais gravadas nas salas. / Acoustic parameters are the criteria that define the acoustic quality of a music hall. The musical audition inside a room is influenced by a group of acoustic impressions that occur at the same time. Each one of such impressions is associated with a particular subjective parameter that is correlated to a measurable physical value. These values are taken as a set of objective parameters that constitute a scientific basis for the acoustical analysis of a music hall. In this work we have conducted both a theoretical and an experimental investigation on the analysis of the most important acoustic parameters for the evaluation of the quality of a music hall. Also, we have done an extensive research on the related bibliography to support our measurement procedures and formal conclusions. We have implemented the necessary technology to obtain the acoustic parameters. We also have determined the most efficient experimental methodology to carry out acoustic measurements and we have applied this methodology to the measurement of six important concert halls. Then we have compared the data related to each hall and performed a critical analysis of this data, increasing our understanding on the meaning and the usefulness of the acoustic parameters. Finally, we have made a subjective jury analysis, correlating the measured acoustic parameters to the impressions about music samples recorded into those concert halls.

We demonstrate a path to hitherto unachievable differential photometric precisions from the ground, both in the optical and near-infrared (NIR), using custom-fabricated beam-shaping diffusers produced using specialized nanofabrication techniques. Such diffusers mold the focal plane image of a star into a broad and stable top-hat shape, minimizing photometric errors due to non-uniform pixel response, atmospheric seeing effects, imperfect guiding, and telescope-induced variable aberrations seen in defocusing. This PSF reshaping significantly increases the achievable dynamic range of our observations, increasing our observing efficiency and thus better averages over scintillation. Diffusers work in both collimated and converging beams. We present diffuser-assisted optical observations demonstrating 62(-16)(+26) ppm precision in 30 minute bins on a nearby bright star 16 Cygni A (V = 5.95) using the ARC 3.5 m telescope-within a factor of similar to 2 of Kepler's photometric precision on the same star. We also show a transit of WASP-85-Ab (V = 11.2) and TRES-3b (V = 12.4), where the residuals bin down to 180(-41)(+66) ppm in 30 minute bins for WASP-85-Ab-a factor of similar to 4 of the precision achieved by the K2 mission on this target-and to 101 ppm for TRES-3b. In the NIR, where diffusers may provide even more significant improvements over the current state of the art, our preliminary tests demonstrated 137(-36)(+64) ppm precision for a K-S = 10.8 star on the 200 inch. Hale Telescope. These photometric precisions match or surpass the expected photometric precisions of TESS for the same magnitude range. This technology is inexpensive, scalable, easily adaptable, and can have an important and immediate impact on the observations of transits and secondary eclipses of exoplanets.

We present the results of a spectroscopic analysis of rotational velocities in 714 M-dwarf stars observed by the SDSS-III Apache Point Galactic Evolution Experiment (APOGEE) survey. We use a template-fitting technique to estimate v sin i while simultaneously estimating log g, [M/H], and T-eff. We conservatively estimate that our detection limit is 8 km s(-1). We compare our results to M-dwarf rotation studies in the literature based on both spectroscopic and photometric measurements. Like other authors, we find an increase in the fraction of rapid rotators with decreasing stellar temperature, exemplified by a sharp increase in rotation near the M4 transition to fully convective stellar interiors, which is consistent with the hypothesis that fully convective stars are unable to shed angular momentum as efficiently as those with radiative cores. We compare a sample of targets observed both by APOGEE and the MEarth transiting planet survey and find no cases where the measured v sin i. and rotation period are physically inconsistent, requiring sin i > 1. We compare our spectroscopic results to the fraction of rotators inferred from photometric surveys and find that while the results are broadly consistent, the photometric surveys exhibit a smaller fraction of rotators beyond the M4 transition by a factor of similar to 2. We discuss possible reasons for this discrepancy. Given our detection limit, our results are consistent with a bimodal distribution in rotation that is seen in photometric surveys.

Context. Post-extreme horizontal branch stars (post-EHB) are helium-shell burning objects evolving away from the EHB and contracting directly towards the white dwarf regime. While the stars forming the EHB have been extensively studied in the past, their hotter and more evolved progeny are not so well characterized. Aims. We perform a comprehensive spectroscopic analysis of four such bright sdO stars, namely Feige 34, Feige 67, AGK+81 degrees 266, and LS II + 18 degrees 9, among which the first three are used as standard stars for flux calibration. Our goal is to determine their atmospheric parameters, chemical properties, and evolutionary status to better understand this class of stars that are en route to become white dwarfs. Methods. We used non-local thermodynamic equilibrium model atmospheres in combination with high quality optical and UV spectra. Photometric data were also used to compute the spectroscopic distances of our stars and to characterize the companion responsible for the infrared excess of Feige 34. Results. The four bright sdO stars have very similar atmospheric parameters with T-eff between 60 000 and 63 000 K and log g (cm s(-2)) in the range 5.9 to 6.1. This places these objects right on the theoretical post-EHB evolutionary tracks. The UV spectra are dominated by strong iron and nickel lines and suggest abundances that are enriched with respect to those of the Sun by factors of 25 and 60. On the other hand, the lighter elements, C, N, O, Mg, Si, P, and S are depleted. The stars have very similar abundances, although AGK + 81 degrees 266 shows differences in its light element abundances. For instance, the helium abundance of this object is 10 times lower than that observed in the other three stars. All our stars show UV spectral lines that require additional line broadening that is consistent with a rotational velocity of about 25 km s(-1). The infrared excess of Feige 34 is well reproduced by a M0 main-sequence companion and the surface area ratio of the two stars suggests that the system is a physical binary. However, the lack of radial velocity variations points towards a low inclination and/or long orbital period. Spectroscopic and HIPPARCOS distances are in good agreement for our three brightest stars. Conclusions. We performed a spectroscopic analysis of four hot sdO stars that are very similar in terms of atmospheric parameters and chemical compositions. The rotation velocities of our stars are significantly higher than what is observed in their immediate progenitors on the EHB, suggesting that angular momentum may be conserved as the stars evolve away from the EHB.

We determine the mass scale of Planck galaxy clusters using gravitational lensing mass measurements from the Cluster Lensing And Supernova survey with Hubble (CLASH). We have compared the lensing masses to the Planck Sunyaev-Zeldovich (SZ) mass proxy for 21 clusters in common, employing a Bayesian analysis to simultaneously fit an idealized CLASH selection function and the distribution between the measured observables and true cluster mass. We used a tiered analysis strategy to explicitly demonstrate the importance of priors on weak lensing mass accuracy. In the case of an assumed constant bias, b(SZ), between true cluster mass, M-500, and the Planck mass proxy, M-PL, our analysis constrains 1 - b(SZ) = 0.73 +/- 0.10 when moderate priors on weak lensing accuracy are used, including a zero-mean Gaussian with standard deviation of 8% to account for possible bias in lensing mass estimations. Our analysis explicitly accounts for possible selection bias effects in this calibration sourced by the CLASH selection function. Our constraint on the cluster mass scale is consistent with recent results from the Weighing the Giants program and the Canadian Cluster Comparison Project. It is also consistent, at 1.34 sigma, with the value needed to reconcile the Planck SZ cluster counts with Planck's base Lambda CDM model fit to the primary cosmic microwave background anisotropies.

No description available.

We describe how to estimate the velocity dispersions of ultradiffuse galaxies (UDGs) using a previously defined galaxy scaling relationship. The method is accurate for the two UDGs with spectroscopically measured dispersions, as well as for ultracompact galaxies, ultrafaint galaxies, and stellar systems with little or no dark matter. This universality means that the relationship can be applied without further knowledge or prejudice regarding the structure of a galaxy. We then estimate the velocity dispersions of UDGs drawn from two published samples and examine the distribution of total masses. We find, in agreement with the previous studies of two individual UDGs, that these systems are dark matter dominated systems, and that they span a range of at least 10(10) < M-200/M-circle dot < 10(12). These galaxies are not, as an entire class, either all dwarfs or all failed L-* galaxies. Estimates of the velocity dispersions can also help identify interesting subsets of UDGs, such as those that are likely to have the largest mass-to-light ratios, for subsequent spectroscopic study.

The non-destructive measurement of deflection basins has come a long way from measuring only maximum deflection or radius of curvature and using empirical relationships in rehabilitation design. New equipment was developed world-wide and analysis techniques moved towards utilising the full deflection basin in fundamental analysis procedures. This author addressed the problem of a proper description of the full deflection basin by doing a detailed literature survey on this subject. Various deflection basin parameters that describe the deflection basin are listed, as well as the various measuring apparatus related to them. The apparatus are all discussed in detail and related to the equipment available in South Africa. The measurement of deflection basins with the road surface deflectometer (RSD) under accelerated testing with the fleet of heavy vehicle simulators (HVSs) are described in detail. An improved data manipulation procedure is proposed which simplifies the calculation of all the deflection basin parameters found in literature. Various models to fit the measured deflection basins are also investigated in an effort to describe the deflection basin in full too. The measured deflection basin parameters of a bitumen, granular, cemented and light structured granular base pavement are discussed in detail as being tested with the fleet of HVS's. It is shown how the deflection basin parameters reflect the structural capacity of the various layers and behaviour states. A more accurate description of the behaviour states is made possible with the proposal of ranges for the various behaviour states for these deflection basins selected. A literature study was carried out to investigate the various analysis procedures that use measured deflection basins as basic input in the characterization of materials. On the basis of this study, linear elastic programmes were used to calculate effective elastic moduli for each pavement layer, using measured deflection basins as input. The possibility to relate typical distress determinants to measured deflection basins were investigated in the literature. Based on this, typical South African flexible pavement structures were analysed mechanistically and typical design curves were established for typical bitumen and. granular base pavements. The effect of overlays were investigated too, resulting in typical overlay design curves. In the final chapter the author endeavours to summarise the research by indicating how deflection basins can be measured and enhance the South African mechanistic rehabilitation design process. Only the latter rehabilitation design procedure is discussed with specific reference to the enhancement of the behaviour state identification, material characterization, analysis procedure and rehabilitation design with measured deflection basin parameters. The author ends off by giving an indication of the future research need in this field of deflection basins. / Thesis (PhD)--University of Pretoria, 2010. / Civil Engineering / unrestricted

The objective of this study was to investigate the growth performance, feed conversion efficiency and other production traits of beef cattle performance tested on the farm. Performance testing records (collected from 2000 to 2004), of 444 bulls comprising of six breeds [viz. Aberdeen Angus (n = 42), Beefmaster (n = 135), Bonsmara (n = 97), Drakensberger (n = 64), Nguni (n = 50) and Simbra (n = 56)] from the eastern Free State, Veld Bull Club (VBC) were obtained and analysed. Bulls were performance tested on the farm (Poortije in Vrede district) for 205 days (16.53 s.d.) and finished-off in a feedlot for 100 days. Upon the completion of the entire test period, the bulls were auctioned. Traits studied were: average daily gain (ADG), Kleiber ratio (KR) and veld feed conversion ratio (VFCR), body conditions score (BCS), muscling score (MS), temperament score (TS), tick count (TC), scrotum circumference (SC) and selling price (SP). An analysis of variance with the General Linear Model (GLM) was used to determine the significance within a breed between years, between breeds within a year, the interaction of year x breed, and breeders (breed x year) for all the dependent variables. Aberdeen Angus bulls showed a significant difference for all traits analysed except for SC and SP. Beefmasters did not only differ in BCS and TS. Bonsmaras differed in all traits analysed except for FWT, SC and SP. Unlike the other breeds, the Drakensberger had more traits that they showed no significant differences viz. IWT, FWT, MS, TS and SP. The Nguni showed significant difference in all traits analysed except for IWT, TS and SC. Finally, the Simbra also did not differ significantly in five of the eleven traits measured viz. FWT, MS, TC, SC and SP. According to these results, there is a significant variation within beef cattle breeds on rangeland in certain performance and other production traits such those measured in this study. This suggests that, although selection for desirable traits within-breed may be slow, the within-breed selection and exploitation has a role to play in improving long-term herd functional efficiency. During the feedlotting period, none of the breeds showed a significant difference in ADG, suggesting that, given a favourable environment, each animal will have an equal opportunity to perform at its optimum genetic potential. This further implies that in a production environment where feed resource is not the limiting factor, higher production efficiency may well be accomplished by each animal. / Dissertation (MSc(Agric): Animal Production Management)--University of Pretoria, 2008. / Animal and Wildlife Sciences / MSc(Agric) / unrestricted