Dynamical star-disk interaction in the young stellar system V354 Mon

The main goal of this work is to characterize the mass accretion and ejection processes of the classical T Tauri star V354 Mon, a member of the young stellar cluster NGC 2264. In March 2008, photometric and spectroscopic observations of V354 Mon were obtained simultaneously with the CoRoT satellite, the 60 cm telescope at the Observat\'orio Pico dos Dias (LNA - Brazil) equipped with a CCD camera and Johnson/Cousins BVRI filters, and the SOPHIE \'echelle spectrograph at the Observatoire de Haute-Provence (CNRS - France). The light curve of V354 Mon shows periodical minima (P = 5.26 +/- 0.50 days) that vary in depth and width at each rotational cycle. From the analysis of the photometric and spectroscopic data, it is possible to identify correlations between the emission line variability and the light-curve modulation of the young system, such as the occurrence of pronounced redshifted absorption in the H_alpha line at the epoch of minimum flux. This is evidence that during photometric minima we see the accretion funnel projected onto the stellar photosphere in our line of sight, implying that the hot spot coincides with the light-curve minima. We applied models of cold and hot spots and a model of occultation by circumstellar material to investigate the source of the observed photometric variations. We conclude that nonuniformly distributed material in the inner part of the circumstellar disk is the main cause of the photometric modulation, which does not exclude the presence of hot and cold spots at the stellar surface. It is believed that the distortion in the inner part of the disk is created by the dynamical interaction between the stellar magnetosphere, inclined with respect to the rotation axis, and the circumstellar disk, as also observed in the classical T Tauri star AA Tau and predicted by magnetohydrodynamical numerical simulations.Comment: Accepted by Astronomy and Astrophysic

Proposição de um índice de produção para bibliotecas com uso do Método MACBETH.

O artigo apresenta o uso de um método multicritério (MACBETH) para propor um índice de produção ponderado para bibliotecas

Confinement of bosonic and spinning particles in braneworlds

In this manuscript we study the confinement of bosonic and spinning test particles in smooth Randall-Sundrum models. For this, we show that it is possible to find an effective potential which describe the motion of the particle over the extra dimension. For the bosonic case it is a known fact that free test particles cannot be localized neither in thin nor thick branes. Recently, a coupling to a scalar field has been used to localize a limited range of masses. Up to now, no mechanism has been found that can trap test particles of any mass over the brane. To solve this, we show that a coupling with the dilaton can trap particles of any mass. Next we analyze the spinning particle. The spin variables $\psi^{P}$ introduces an interaction with the curvature Riemann tensor. This introduces a correction to the effective potential. By analyzing it, we find that the spinning particle can be localized at a position different of the brane. We also show that a spinning particle over the brane can escape to infinity. Therefore, we can conclude that free bosonic and spinning particles are not trapped to the brane

Desempenho produtivo de fêmeas das raças Canchim e Nelore. III. Produção de leite.

Comparar a produtividade de leite de vacas primiparas das raças Canchim e Nelore

Dynamical Mass Constraints on Low-Mass Pre-Main-Sequence Stellar Evolutionary Tracks: An Eclipsing Binary in Orion with a 1.0 Msun Primary and an 0.7 Msun Secondary

We report the discovery of a double-lined, spectroscopic, eclipsing binary in the Orion star-forming region. We analyze the system spectroscopically and photometrically to empirically determine precise, distance-independent masses, radii, effective temperatures, and luminosities for both components. The measured masses for the primary and secondary, accurate to ~1%, are 1.01 Msun and 0.73 Msun, respectively; thus the primary is a definitive pre-main-sequence solar analog, and the secondary is the lowest-mass star yet discovered among pre-main-sequence eclipsing binary systems. We use these fundamental measurements to test the predictions of pre-main-sequence stellar evolutionary tracks. None of the models we examined correctly predict the masses of the two components simultaneously, and we implicate differences between the theoretical and empirical effective temperature scales for this failing. All of the models predict the observed slope of the mass-radius relationship reasonably well, though the observations tend to favor models with low convection efficiencies. Indeed, considering our newly determined mass measurements together with other dynamical mass measurements of pre-main-sequence stars in the literature, as well as measurements of Li abundances in these stars, we show that the data strongly favor evolutionary models with inefficient convection in the stellar interior, even though such models cannot reproduce the properties of the present-day Sun.Comment: Accepted by Ap

Análise de dinâmica de uso e de desempenho: o caso do web site da Embrapa Monitoramento por Satélite

A Embrapa Monitoramento por Satélite, há mais de uma década, utiliza a Internet como meio de difusão de resultados de pesquisa e de interação com clientes, parceiros e usuários. Com intuito de avaliar o uso do web site por esse público e o desempenho do sistema de comunicação eletrônica envolvido, tem-se utilizado o programa Webalizer, que monitora e elabora estatísticas de entradas e saídas do sistema, com base na análise de arquivos de log. Com os indicadores contabilizados pelo programa foi possível avaliar aspectos sobre a origem dos acessos, as ações executadas pelos usuários e sobre aspectos do desempenho do sistema em termos de respostas enviadas às solicitações dos usuários. Os resultados podem possibilitar a remodelagem do web site, de modo a melhorar a dinâmica de interação instituição-usuário e promover o desenvolvimento de uma abordagem própria de análise de logs

Towars web site user's profile: log file analysis.

The Internet is a remote, innovative, extremely dynamic and widely accessible communication medium. As in all other human communication formats, we observe the development and adoption of its own language, inherent to its multimedia aspects. The Embrapa Satellite Monitoring is using the Internet as a dissemination medium of its research results and interaction with clients, partners and web site users for more than one decade. In order to evaluate the web site usage and performance of the e-communication system the Webalizer software has been used to track and to calculate statistics based on web server log file analysis. The objective of the study is to analyze the data and evaluate the indicators related to requests origin (search string, country, time), actions performed by users (entry pages, agents) and system performance (error messages). It will help to remodel the web site design to improve the interaction dynamics and also develop a customized log file analyser. This tool would retrieve coherent and real information

Monitoramento e determinação do nível de ação do ácaro-rajado na cultura da uva.

bitstream/CPATSA/26987/1/CTE71.pd

Uso e desempenho de web sites: um estudo de caso.

A Internet é um meio de comunicação remota, inovador, extremamente dinâmico e, cada vez mais, amplamente acessível, que tem adotado uma linguagem própria, inerente à sua natureza multimídia. A Embrapa Monitoramento por Satélite, há mais de uma década, utiliza a Internet como meio de difusão de resultados de pesquisa e de interação com clientes, parceiros e usuários. Com intuito de avaliar o uso do web site por esse público e o desempenho do sistema de comunicação eletrônica envolvido, tem-se utilizado o programa Webalizer que monitora e elabora estatísticas de entradas e saídas do sistema, com base na análise de arquivos de log. Através dos indicadores pelo programa foi possível avaliar aspectos sobre a origem dos acessos, as ações executadas pelos usuários e sobre aspectos do desempenho do sistema em termos de respostas enviadas às solicitações dos usuários. Os resultados podem possibilitar a remodelagem do web site, de modo a melhorar a dinâmica de interação instituição-usuário e promover o desenvolvimento de uma abordagem própria de análise de logs