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Research paper thumbnail of Evolutionary study of the Be star 28 Tau

Proceedings of The International Astronomical Union, 2011

We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The... more We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The photometric data during the absence of its envelope in 1921 have been used to determine the effective temperature and luminosity of the star at the main sequence of the HR diagram. From an evolutionary model, we found that the mass and radius

Research paper thumbnail of Evolutionary study of the Be star 28 Tau

Proceedings of The International Astronomical Union, 2011

We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The... more We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The photometric data during the absence of its envelope in 1921 have been used to determine the effective temperature and luminosity of the star at the main sequence of the HR diagram. From an evolutionary model, we found that the mass and radius

Research paper thumbnail of Evolutionary study of the Be star 28 Tau

Proceedings of The International Astronomical Union, 2011

We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The... more We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The photometric data during the absence of its envelope in 1921 have been used to determine the effective temperature and luminosity of the star at the main sequence of the HR diagram. From an evolutionary model, we found that the mass and radius

Research paper thumbnail of Evolutionary study of the Be star 28 Tau

Proceedings of The International Astronomical Union, 2011

We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The... more We present an evolutionary study of 28 Tau, a Be star, in connection with its rapid rotation. The photometric data during the absence of its envelope in 1921 have been used to determine the effective temperature and luminosity of the star at the main sequence of the HR diagram. From an evolutionary model, we found that the mass and radius

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