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Para a confecção deste modelo foi utilizado a última versão (one.9.six) do pacote de courses \textit abnTeX2 que segue as normas da Associação Brasileira de Normas Técnicas. A elaboração de uma monografia, dissertação ou tese pode ser feita sobrescrevendo o conteúdo deste modelo. Modelo, Monografia de qualificação, Dissertação, Tese, Latex % resumo em INGLÊS
termo midia da língua inglesa, é um silogismo importado daquela língua. Sua origem é a mesma da língua
Photometric variability is without doubt one of the principal characteristics of younger stellar objects and exploring its particularities in several wavelengths might present insights on the ongoing Actual physical processes at work in this sort of objects. The most typical source of photometric variability in youthful stars will be the brightness modulation because of the rotation of a noticed stellar surface area. Such a variability permits the measurement of rotational durations in younger stars. In the final a long time, the early pre-most important sequence stellar rotational evolution image has been constrained by reports targeting diverse young areas at a variety of ages. Observational reports advise a dependence of rotation with mass, and for a few mass ranges a relationship amongst rotation and the presence of the circumstellar disc. Not nevertheless totally explored, even though, is definitely the position of environmental conditions about the stellar rotational regulation. In this particular thesis, we explored the incidence and primary features of near-infrared variability in younger stars in The large OB association Cygnus OB2, and that is 1.four kpc away from the Solar. For objects with periodic variability that can be connected with stellar rotation, we investigated the rotational Houses of Cygnus OB2 members. To the sample of rotational durations evaluated, we tackled inquiries concerning the impact of natural environment Qualities to the pre-principal sequence rotational evolution. We investigated JHK-band variability of 5083 prospect associates (24% of which happen to be disc-bearing stars), utilizing knowledge observed While using the vast-subject camera (WFCAM) of the UK Infrared Telescope (UKIRT) on Mauna Kea, Hawaii. A complete of 112 evenings had been noticed, spanning 217 days. The sample researched is unfold in excess of a area of 0.78 squared degrees. The choice of variable stars was carried out employing Stetson variability index, and 60% of The celebrities within the sample have been observed to be variable In line with this criterion.
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We investigated the light-curve Dissertação de Mestrado morphology, along with the variants in the colour-colour and colour-magnitude diagrams for JHK-bands, and once the variability was hugely correlated in several bands and colors, the slopes produced by the variations within these kinds of diagrams were being estimated. These slopes had been when compared with the slopes predicted within the models describing Bodily mechanisms dependable by the variability in younger stars, plus the results in of variability ended up investigated. Period research was carried out using Lomb-Scargle periodogram for Monografias Prontas intervals in between 0.eighty three-forty five times. Period detections had been verified by utilizing Wrong Alarme Chance concentrations, the Saunders statistics, string/rope length technique, and visual verification of folded mild curves. We determined 1224 periodic variable stars. Monte Carlo simulations were being performed so that you can Appraise completeness and contamination from the periodic sample, outside of which 894 measured periods ended up considered as responsible. Our examine was considered resonably finish for durations among two and 30 times. The overall scenario for your rotational evolution of youthful stars seen in other areas is verified by Cygnus OB2 interval distributions, with disc-bearing stars rotating on typical slower than stars without the need of discs. A mass-rotation dependence was also verified, but as in NGC 6530, quite very low mass stars (M < 0.four Msun) are rotating on normal slower than better mass stars (0.four Msun < M < one.four Msun). We noticed an surplus of sluggish rotators Among the many decrease mass populace. The disc and mass-rotation relationship was also analysed by taking into account the incident UV radiation arising from O stars in the association. Results appropriate with the disc-locking state of affairs were confirmed for stars with reduced UV incidence, but no statistical important relation concerning rotation and disc existence was confirmed for stars with significant UV incidence, suggesting that large stars may have a vital position on regulating the rotation of close by very low mass stars.
% Tanto na capa quanto nas folhas de rosto apenas a primeira letra da primeira palavra (ou nomes próprios) devem estar em letra maiúscula, todas as demais devem ser em letra minúscula.
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\start anexosenv \chapter Páginas interessantes na Web \label chapter:paginas-interessantes \input tex/annex/paginas-interessantes \finish anexosenv
\textoresumo[brazil] Este trabalho é um breve modelo para a escrita de monografias de qualificação, dissertações e teses utilizando o ambiente \LaTeX, de acordo com as normas exigidas pelo Instituto de Ciências Matemáticas e de Computação (ICMC), da Universidade de São Paulo (USP)