Reinforcing the link between the double red clump and the X-shaped bulge of the Milky Way

The finding of a double red clump in the luminosity function of the Milky Way bulge has been interpreted as evidence for an X-shaped structure. Recently, an alternative explanation has been suggested, where the double red clump is an effect of multiple stellar populations in a classical spheroid. In this Letter we provide an observational assessment of this scenario and show that it is not consistent with the behaviour of the red clump across different lines of sight, particularly at high distances from the Galactic plane. Instead, we confirm that the shape of the red clump magnitude distribution closely follows the distance distribution expected for an X-shaped bulge at critical Galactic latitudes. We also emphasize some key observational properties of the bulge red clump that should not be neglected in the search for alternative scenarios

Beryllium abundances in stars hosting giant planets

We have derived beryllium abundances in a wide sample of stars hosting planets, with spectral types in the range F7V-K0V, aimed at studying in detail the effects of the presence of planets on the structure and evolution of the associated stars. Predictions from current models are compared with the derived abundances and suggestions are provided to explain the observed inconsistencies. We show that while still not clear, the results suggest that theoretical models may have to be revised for stars with Teff<5500K. On the other hand, a comparison between planet host and non-planet host stars shows no clear difference between both populations. Although preliminary, this result favors a ``primordial'' origin for the metallicity ``excess'' observed for the planetary host stars. Under this assumption, i.e. that there would be no differences between stars with and without giant planets, the light element depletion pattern of our sample of stars may also be used to further investigate and constraint Li and Be depletion mechanisms.Comment: A&A in press -- accepted on the 22/02/2002 (11 pages, 6 figures included

Bending reinforcement of timber beams with composite carbon fiber and basalt fiber materials

En el presente trabajo se lleva a cabo un estudio basado en datos obtenidos experimentalmente mediante el ensayo a flexión de vigas de madera de pino silvestre reforzadas con materiales compuestos. Las fibras que componen los tejidos utilizados para la ejecución de los refuerzos son de basalto y de carbono. En el caso de los compuestos de fibra de basalto se aplican en distintos gramajes, y los de carbono en tejido unidireccional y bidireccional. El material compuesto se realizó in situ, simultáneamente a la ejecución del refuerzo. Se aplicaron en una y en dos capas, según el caso, y la forma de colocación fue en ?U?, adhiriéndose al canto inferior y a las caras laterales de la viga mediante resina o mortero epoxi. Se analiza el comportamiento de las vigas según las variables de refuerzo aplicadas y se comparan con los resultados de vigas ensayadas sin reforzar. Con este trabajo queda demostrado el buen funcionamiento del FRP de fibra de basalto aplicado en el refuerzo de vigas de madera y de los tejidos de carbono bidireccionales con respecto a los unidireccionales

Ecosocioeconomics applied to urban freight by bicycle and motorcycle in the city of Curitiba, Brazil

The aim of this work is to compare the logistics of urban light weight delivery by motorcycle and bicycle. To this purpose, a case study in the city of Curitiba, Brazil, was chosen. City planning demands alternative solutions to everyday problems, among which use of urban space and mobility are relevant due to fast and rather chaotic growing. Urban mobility −a complex network comprising a variety of actors and areas; has social, economic and environmental impacts that might be underestimated in planning and implementation of actions. So far, and for the case studied here, urban planning for light weight delivery has not included externalities, but rather focused on technical issues on logistics and urban traffic. For instance, the rates of dead and disability from accidents on this mobility are currently very high. In the present research, two light weight deliveries actually used in Curitiba were compared: motorbikes and bicycles. The analysis is based on the methodology of the eco-socio-economy of organizations. This approach considers the complexity of subsystems linked, and the effectiveness beyond the organization but on the social demands in the urban territory. The use of bicycles was studied using data from EcoBike, analyzed here and compared to the generic case of deliveries by motorbikes. Indicators for accidents (with and without death), fossil energy used, CO2 emissions, and operative costs were obtained and compared. The indicators assessed favour the use of bicycles over motorbikes.Fil: García, M.. Pontifícia Universidade Católica do Paraná; BrasilFil: Sampaio, C. A. C.. Pontifícia Universidade Católica do Paraná; BrasilFil: Gonzalez, Alejandro Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Patagonia Norte. Instituto de Investigación en Biodiversidad y Medioambiente; Argentina. Universidad Nacional del Comahue; Argentin

Estudio de la resistencia de vigas de madera reforzadas con FRP de tejidos unidireccionales y bidireccionales de fibra de carbono

En este trabajo se realiza un estudio experimental del comportamiento de veinte vigas de madera aserrada de pino silvestre para uso estructural, de dimensiones 155x75x1090mm y reforzadas con materiales compuestos de fibra de carbono. La procedencia de la madera es el aserradero de Valsaín. Los ensayos se han realizado en el Laboratorio de Materiales de Construcción de la Escuela Universitaria de Arquitectura Técnica de Madrid con una máquina de ensayos Universal. El objetivo del trabajo es el análisis del comportamiento a flexión de las piezas ensayadas reforzadas con materiales compuestos de fibra de carbono realizados con tejidos unidireccionales y bidireccionales. De las veinte vigas ensayadas nueve fueron sin reforzar y el resto se reforzaron con el refuerzo en forma de ?U?, adhiriendo el material compuesto a la cara inferior y los laterales de las vigas, hasta una altura de la mitad del canto. Para la realización de los FRP se han empleado tejidos de fibra de carbono unidireccionales y bidireccionales. El gramaje de los tejidos unidireccionales es de 300gr/m2 y se ha aplicado en una capa. Los tejidos bidireccionales utilizados tienen dos gramajes distintos, 160gr/m2 y 210gr/m2. Éstos últimos se han aplicado en una y en dos capas. Las nueve vigas ensayadas sin reforzar han servido como testigo para analizar el aumento de la capacidad de carga de las vigas reforzadas. A partir de los datos facilitados por el software se asociado a la máquina de ensayos se trazaron los gráficos carga-desplazamiento, con el fin de analizar las cargas máximas de rotura alcanzadas, desplazamientos y rigidez de las piezas. Posteriormente se realiza un análisis analítico hallando los valores medio de las cargas de rotura y los desplazamientos, realizando una comparación entre los datos obtenidos para las vigas sin reforzar y las reforzadas con los distintos sistemas. En las conclusiones se presentan los resultados del análisis realizado, estudiando el incremento de la capacidad de carga de las vigas reforzadas con respecto a las no reforzadas, y comparando entre sí el funcionamiento de los refuerzos aplicados

Are beryllium abundances anomalous in stars with giant planets?

In this paper we present beryllium (Be) abundances in a large sample of 41 extra-solar planet host stars, and for 29 stars without any known planetary-mass companion, spanning a large range of effective temperatures. The Be abundances were derived through spectral synthesis done in standard Local Thermodynamic Equilibrium, using spectra obtained with various instruments. The results seem to confirm that overall, planet-host stars have ``normal'' Be abundances, although a small, but not significant, difference might be present. This result is discussed, and we show that this difference is probably not due to any stellar ``pollution'' events. In other words, our results support the idea that the high-metal content of planet-host stars has, overall, a ``primordial'' origin. However, we also find a small subset of planet-host late-F and early-G dwarfs that might have higher than average Be abundances. The reason for the offset is not clear, and might be related either to the engulfment of planetary material, to galactic chemical evolution effects, or to stellar-mass differences for stars of similar temperature.Comment: 15 pages, 9 figures, accepted for publication in Astronomy & Astrophysic

Conceptual design of the ITER fast-ion loss detector

et al.A conceptual design of a reciprocating fast-ion loss detector for ITER has been developed and is presented here. Fast-ion orbit simulations in a 3D magnetic equilibrium and up-to-date first wall have been carried out to revise the measurement requirements for the lost alpha monitor in ITER. In agreement with recent observations, the simulations presented here suggest that a pitch-angle resolution of ∼5° might be necessary to identify the loss mechanisms. Synthetic measurements including realistic lost alpha-particle as well as neutron and gamma fluxes predict scintillator signal-to-noise levels measurable with standard light acquisition systems with the detector aperture at ∼11 cm outside of the diagnostic first wall. At measurement position, heat load on detector head is comparable to that in present devices.This research was supported in part by the Spanish Ministry of Economy and Competitiveness (Grant Nos. RYC2011-09152, FIS2015-69362-P, and ENE2012- 31087) and the Marie Curie FP7 Integration Grant (No. PCIG11-GA2012-321455).Peer Reviewe

Influencia del origen del haba sobre el valor nutricional de la harina de soja

La harina de soja (HS) es la principal fuente de proteína en piensos para animales monogástricos. La mayor parte de las HS utilizadas en Europa proceden del continente Americano, en particular de Argentina (ARG), Brasil (BRA) y Estados Unidos (USA). Aunque la composición y valor nutricional de las HS varía entre países de origen (Grieshop et al., 2003; De Coca et al., 2008; 2010; Valencia et al., 2008), las tablas de composición de alimentos (NRC, 1998; FEDNA, 2010) clasifican las HS en función de su contenido en PB, sin tener en cuenta ni el origen ni las condiciones del procesado. En un trabajo anterior Mateos et al. (2009) se presentaron los resultados obtenidos de una colección de 262 muestras de HS recolectadas en las cosechas de los años 2007 y 2008 procedentes de estos tres países. Dependiendo de la variable considerada, el número de muestras analizadas varió entre 50 y 262. El presente trabajo tuvo como objetivo completar los análisis y complementar los resultados anteriores en relación con la composición química, el valor nutricional y la calidad de la PB de la HS con nuevas muestras procedentes de las cosechas de los años 2009 y 2010

Say what? : On the transmission of acoustic signals in a Neotropical green city

Cities do not only represent noisy systems, but also limit acoustic communication given the complex array of artificial structures through which signals can be trapped or obscured. In this study we performed a field experiment to evaluate the loss of energy of a standardized acoustic emission (generated with notes and a call of the Clay-colored Thrush - Turdus grayi). For this, we emitted the acoustic signal and recovered it at increasing radial distances from 26 fixed emission points (i.e., 10 m, 20 m, 40 m, 80 m, 120 m, 160 m) located across the city of Xalapa (Mexico). Our results show that the emitted signal was not recorded beyond 80 m from the emission point. The number and height of the assessed physical obstacles between the emitted signal and the receiving equipment showed to drive our main result, with built elements representing a major barrier than vegetation ones in terms of the recovered energy of the emitted signal. Interestingly, we found that, for both types of physical obstacles, a height of similar to 7 m was a common threshold influencing the recovered energy of the emitted signal.Peer reviewe