Master in Astronomy from the Institute of Astronomy, Geophysics and Atmospheric Sciences at USP. Currently a member of the BeACoN study group at IAG-USP, focused on the study of Be stars.Twice Student Representative of the Technical Administrative Council of IAG-USP (2019-2021). Student Representative on the IAG-USP Postgraduate Committee (2022-2023).Former FAPESP Scientific Initiation Fellow, in the stellar sub-area - Be Stars. Brief experience in teaching. Fluent English (B2). Experience in High Performance Computing.Advanced knowledge of Python. Intermediate programming in C, R and CUDA. Experience in scientific outreach. (Source: Lattes Curriculum)
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Classical Be stars are fast rotating, non super-giant, B-type stars that have (or had at some moment) emission lines in their spectra. This emission feature is due to the reprocessing of ultraviolet light by a viscous decretion disk, ejected from the stellar equator by a still unknown mechanism that involves the near-critical rotation of the central star and maybe radial and non-radial pu…
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