Age of the magnetically active WW Psa and TX Psa members of the β Pictoris association
Context. There are a variety of different techniques available to estimate the ages of pre-main-sequence stars. Components of physical pairs, thanks to their strict coevality and the mass difference, such as the binary system analyzed in this paper, are best suited to test the effectiveness of these...
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2017
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v601_n_p_Messina http://hdl.handle.net/20.500.12110/paper_00046361_v601_n_p_Messina |
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