MML 53: a new low-mass, pre-main sequence eclipsing binary in the Upper Centaurus-Lupus region discovered by SuperWASP

We announce the discovery of a new low-mass, pre-main sequence eclipsing binary, MML 53. Previous observations of MML 53 found it to be a pre-main sequence spectroscopic multiple associated with the 15-22 Myr Upper Centaurus-Lupus cluster. We identify the object as an eclipsing binary for the first time through the analysis of multiple seasons of time series photometry from the SuperWASP transiting planet survey. Re-analysis of a single archive spectrum shows MML 53 to be a spatially unresolved triple system of young stars which all exhibit significant lithium absorption. Two of the components comprise an eclipsing binary with period, P = 2.097891(6) ± 0.000005 and mass ratio, q ~ 0.8. Here, we present the analysis of the discovery data.

Regiões de estabilidade no ambiente de um sistema de asteroide triplo

This work was developed from the study by Araujo, R.A.N. et al. Stability regions around the components of the triple system 2001 SN263. (Monthly Notices Of The Royal Astronomical Society, 2012, v. 423(4), 3058-3073 p.) where it was studied the stable and unstable regions system (2001 SN263), which is a triple asteroid system, and these are celestial orbiting our sun. Being close to the Earth is characterized as NEA (Near-Earth Asteroids), asteroids and which periodically approach the Earth's orbit, given that there is great interest in the study and exploitation of these objects, it is the key can carry features that contribute to better understand the process of formation of our solar system. Study the dynamics of bodies that govern those systems proves to be greatly attractive because of the mutual gravitational perturbation of bodies and also by external disturbances. Recently, NEA 2001 SN263 was chosen as a target of Aster mission where a probe is sent for this triple system, appearing therefore the need for obtaining information for characterizing stable regions internal and external to the system, with respect to the effects of radiation pressure. First, this study demonstrated that the integrator used showed satisfactory results of the orbital evolution of bodies in accordance with previous studies and also the characterization of stable and unstable regions brought similar results to the study by Araujo et al. (2012). From these results it was possible to carry out the implementation of the radiation pressure in the system in 2001 SN263, in a region close to the central body, where the simulations were carried out, which brought as a result that the regions before being characterized as stable in unstable true for small particles size from 1 to 5 micrometers. So the next orbital region to the central body and the ... ( Complete abstract click electronic access below)

Regiões de estabilidade no ambiente de um sistema de asteroide triplo

This work was developed from the study by Araujo, R.A.N. et al. Stability regions around the components of the triple system 2001 SN263. (Monthly Notices Of The Royal Astronomical Society, 2012, v. 423(4), 3058-3073 p.) where it was studied the stable and unstable regions system (2001 SN263), which is a triple asteroid system, and these are celestial orbiting our sun. Being close to the Earth is characterized as NEA (Near-Earth Asteroids), asteroids and which periodically approach the Earth's orbit, given that there is great interest in the study and exploitation of these objects, it is the key can carry features that contribute to better understand the process of formation of our solar system. Study the dynamics of bodies that govern those systems proves to be greatly attractive because of the mutual gravitational perturbation of bodies and also by external disturbances. Recently, NEA 2001 SN263 was chosen as a target of Aster mission where a probe is sent for this triple system, appearing therefore the need for obtaining information for characterizing stable regions internal and external to the system, with respect to the effects of radiation pressure. First, this study demonstrated that the integrator used showed satisfactory results of the orbital evolution of bodies in accordance with previous studies and also the characterization of stable and unstable regions brought similar results to the study by Araujo et al. (2012). From these results it was possible to carry out the implementation of the radiation pressure in the system in 2001 SN263, in a region close to the central body, where the simulations were carried out, which brought as a result that the regions before being characterized as stable in unstable true for small particles size from 1 to 5 micrometers. So the next orbital region to the central body and the ... ( Complete abstract click electronic access below)

Malcev dialgebras

We apply Kolesnikov's algorithm to obtain a variety of nonassociative algebras defined by right anticommutativity and a "noncommutative" version of the Malcev identity. We use computer algebra to verify that these identities are equivalent to the identities of degree up to 4 satisfied by the dicommutator in every alternative dialgebra. We extend these computations to show that any special identity for Malcev dialgebras must have degree at least 7. Finally, we introduce a trilinear operation which makes any Malcev dialgebra into a Leibniz triple system.

The CODE MGEX orbit and clock solution

The Center for Orbit Determination in Europe (CODE) is contributing as a global Analysis center to the International GNSS Service (IGS) since many years. The processing of GPS and GLONASS data is well established in CODE’s ultra-rapid, rapid, and final product lines. With the introduction of new signals for the established and new GNSS, new challenges and opportunities are arising for the GNSS data management and processing. The IGS started the Multi-GNSS-EXperiment (MGEX) in 2012 in order to gain first experience with the new data formats and to develop new strategies for making optimal use of these additional measurements. CODE has started to contribute to IGS MGEX with a consistent, rigorously combined triple-system orbit solution (GPS, GLONASS, and Galileo). SLR residuals for the computed Galileo satellite orbits are of the order of 10 cm. Furthermore CODE established a GPS and Galileo clock solution. A quality assessment shows that these experimental orbit and clock products allow even a Galileo-only precise point positioning (PPP) with accuracies on the decimeter- (static PPP) to meter-level (kinematic PPP) for selected stations.

La catedral de Ávila : evolución constructiva y análisis estructural

Esta tesis se enmarca en el ámbito de la Historia de la Construcción, se estudia la Catedral de Ávila desde un punto de vista técnico, necesario para completar la visión que de esta catedral se tenía. La interpretación de la documentación de archivo, que se encontraba dispersa e inconexa, ha permitido realizar una cronología revisada y completa de las campañas constructivas para el conjunto de la Catedral, desde el siglo XI al XXI. Mediante el análisis de los Contratos de Obra e Informes, se ha puesto de relieve conocimientos de técnicas constructivas medievales. Se plantean dos hipótesis para el orden en el proceso constructivo. En la zona del Cimorro, en relación con la supresión de la tribuna, colocación de los arbotantes y construcción de la fortificación y triple almenado. En el cuerpo de las naves, referida a la posible existencia de una tribuna, colocación del sistema de contrarresto que vemos actualmente y misión del arco entibo del coro. Se ha analizado la estabilidad estructural de la Catedral bajo el marco teórico del Análisis Límite para Estructuras de Fábrica, utilizando la restitución gráfica procedente del levantamiento topográfico realizado. Estos análisis han servido como comprobación de las hipótesis planteadas, por realizarse tanto para la situación actual como para las diferentes campañas constructivas propuestas. Se ha comprobado la validez de las reglas geométricas tradicionales para el análisis de la estructuras de fábrica en los elementos principales de la estructura gótica. Esta tesis incrementa el conocimiento de la historia mecánica del edificio interpretando el funcionamiento mecánico de sus arbotantes, proyectados de forma atípica, y la colocación de los arcos entibo y codales para conseguir la estabilidad del conjunto. La tesis cuenta con un anexo que recopila una extensa documentación gráfica: planimetría, iconografía y fotografía histórica; la trascripción inédita del Contrato de obra para la Capilla de San Segundo y un anexo de cálculo de la zona del Cimorro y del Cuerpo de Naves. This thesis aims to the field of Construction History. The Cathedral of Ávila is studied from a technical point of view, which was necessary to complete the existing knowledge about this Cathedral. The interpretation of archive documentation, which was disperse and unconnected before this work, has allowed the proposal of a revised and complete chronology of the diverse building stages of the Cathedral, dating from the XI century to the XXI century. The analysis of work contracts and of reports has revealed knowledge of medieval construction techniques. Two hypotheses are presented about the order in the construction process. The first hypothesis concerning the destruction of the tribune, the placing of the flying buttress and the building of the fortification and triple system of battlement in the area of the “Cimorro”. The second hypothesis regarding the naves: the possible existence of a tribune, the placing of the system of counterthrust, which can currently be seen, and the function of the “entibo” arch in the choir. The Structural Stability of the Cathedral has been analysed within the theoretical Framework of Limit Analysis to Masonry Structure, by using of the drawing proceeding from our lifting topographical. These analyses have proven the presented hypotheses, since they have been applied to the current situation as well as to the several building stage proposed in the chronology. The validity of the traditional geometric rules for the analysis of the masonry structure in the core elements of Gothic structures has been verified. This thesis increases the knowledge of the mechanical history of the building by interpreting the mechanical working of the flying buttress in an atypical arrangement and the placing of the “entibo” arch and “codal” arch in order to obtain the stability of the monument. The thesis incorporates supplementary material which can be categorized in three groups: 1) extensive graphic documentation (planning, iconography and history photography); 2) the hitherto unknown transcription of the “CONTRATO DE OBRA PARA LA CAPILLA DE SAN SEGUNDO”; 3) an appendix of Analysis of Calculation for the “Cimorro” and the naves.

Generalizations of Cole's Systems

There are four resolvable Steiner triple systems on fifteen elements. Some generalizations of these systems are presented here.

Some generalization of Desargues and Veronese configurations

2000 Mathematics Subject Classification: 51E14, 51E30.

Mean motion resonances and the stability of a circumbinary disk in a triple stellar system

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Planet formation in a triple stellar system: implications of the third star's orbital inclination

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

Implementation of a triple modular redundant FPGA based safety critical system for reliable software execution

This paper describes the implementation of a TMR (Triple Modular Redundant) microprocessor system on a FPGA. The system exhibits true redundancy in that three instances of the same processor system (both software and hardware) are executed in parallel. The described system uses software to control external peripherals and a voter is used to output correct results. An error indication is asserted whenever two of the three outputs match or all three outputs disagree. The software has been implemented to conform to a particular safety critical coding guideline/standard which is popular in industry. The system was verified by injecting various faults into it.

A decision support system for sustainable urban development : the integrated land use and transportation indexing model

The broad definition of sustainable development at the early stage of its introduction has caused confusion and hesitation among local authorities and planning professionals. The main difficulties are experience in employing loosely-defined principles of sustainable development in setting policies and goals. The question of how this theory/rhetoric-practice gap could be filled will be the theme of this study. One of the widely employed sustainability accounting approaches by governmental organisations, triple bottom line, and applicability of this approach to sustainable urban development policies will be examined. When incorporating triple bottom line considerations with the environmental impact assessment techniques, the framework of GIS-based decision support system that helps decision-makers in selecting policy option according to the economic, environmental and social impacts will be introduced. In order to embrace sustainable urban development policy considerations, the relationship between urban form, travel pattern and socio-economic attributes should be clarified. This clarification associated with other input decision support systems will picture the holistic state of the urban settings in terms of sustainability. In this study, grid-based indexing methodology will be employed to visualise the degree of compatibility of selected scenarios with the designated sustainable urban future. In addition, this tool will provide valuable knowledge about the spatial dimension of the sustainable development. It will also give fine details about the possible impacts of urban development proposals by employing disaggregated spatial data analysis (e.g. land-use, transportation, urban services, population density, pollution, etc.). The visualisation capacity of this tool will help decision makers and other stakeholders compare and select alternative of future urban developments.