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Vol. 49 No. 1 (2017)
,
Contributions
Vol. 49 No. 1 (2017)
Contributions
Late O Giants and the Weak Wind Problem
de Almeida E. S. G.
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Marcolino Wagner L. F.
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Pereira Claudio B.
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de Almeida E. S. G.
Laboratoire Lagrange, UMR 7293, Université de Nice-Sophia Antipolis, CNRS, Observatoire de la Côte d'Azur, 06108 Nice, France
0000-0003-1738-7662
Marcolino Wagner L. F.
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Pereira Claudio B.
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PDF
PDF
Keywords
stars: early-type
stars: fundamental parameters
stars: winds
outflows
stars: mass-loss
How to Cite
Late O Giants and the Weak Wind Problem. (2017).
Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias
,
49
(1), 82-82.
https://astronomia.unam.mx/journals/rmxac/article/view/2017rmxac..49...82d
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Abstract
We analysed O giants through UV and optical spectroscopy using the code CMFGEN. We conclude that these stars show weak winds and are at the transition region in luminosity for such issue.
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