In this thesis, Oscar Hernán Ramírez Agudelo presents the quantitative analysis of massive O-type stars in the 30 Doradus region (also known as the Tarantula Nebula) of the Large Magellanic Cloud. During his research he examined the stellar rotational properties of spectroscopic single and binary stars in 30 Doradus and looked at the properties of O-type giants, bright giants, and supergiants.
Mr O.H. Ramírez Agudelo: Properties of Massive Stars in the Tarantula Nebula
Prof. A. de Koter ans Prof. L.B.F.M. Waters.
Dr H. Sana