Sistemde Tek Faz–Toprak Arızasında Arıza Yeri Bulma ve Ġzolasyonu

Uma das perspectivas de nosso trabalho ´e observar o comportamento da abundˆancia de outros elementos qu´ımicos. Al´em de entender qual o papel da rota¸c˜ao na f´ısica que regula o comportamento da abundˆancia de l´ıtio e da atividade cromosf´erica das estrelas an´alogas e gˆemeas solares. Procurar entender tamb´em qual ´e a f´ısica que governa a emiss˜ao de raio- X no processo de evolu¸c˜ao estelar. Outro ponto a ser explorado, ´e ampliar nossa pesquisa, no sentido de acrescentar medidas do campo magn´etico para estrelas gˆemeas e an´alogas

CAP´ITULO 5. CONCLUS ˜OES E PERSPECTIVAS

solares. Devemos destacar a utiliza¸c˜ao dos recentes dados obtidos pelas miss˜oes espaciais CoRoT e Kepler. Neste sentido um primeiro artigo encontra-se em fase de submiss˜ao.

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Apˆendice A

Abaixo, apresentamos as fontes referentes aos valores da abundˆancia de l´ıtio e per´ıodo de rota¸c˜ao das estrelas de nossa amostra.

• Israelian, G., et al. 2004, A&A, 414, 601 • Ramirez, I., et al. 2012 ApJ, 756, 46 • Sousa, S. G., et al. 2010, A&A, 512L, 5 • Wright, N, J., et al. 2011, ApJ, 743, 48