Graduate student, attending since August 2022 the PhD in Astronomy, with emphasis on Stellar Astrophysics, at the Institute of Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo (IAG/USP). Undergraduated in February 2022 in the Bachelor of Astronomy at IAG/USP and in July 2022 in the Bachelor of Physics at the Institute of Physics at USP (IF/USP). He did a scientific initiation in the area of Stellar Astrophysics since 2019 studying young stars. Developed a Scientific-Academic Tutorship with the theme of the study focused on the physical conditions in the stellar interiors and their role in the formation of spectral lines (2018-2019). He was a member of the IAG Junior institution (2018). Completed high school at the Technical State School of São Paulo (ETESP, 2015 - 2017). Worked as assistant professor in the area of Stellar Astrophysics during the first semester of 2022. (Source: Lattes Curriculum)
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The in-depth knowledge of the star formation scenario in OB Associations can bring important clues to better understand the structure and evolution of the Galaxy. In particular, the Canis Major OB1/R1 region, which contains hundreds of young stars associated with the bubble-like distribution named "CMa shell", is very interesting for exploring the supernova (SN) effect on star forming…
We will perform optical spectral lines measurements of T Tauri stars aiming to estimate stellar parameters such as effective temperature, gravity and metallicity. One of the goals is to provide to the student the learning of statistical physics involved in the formation and characterization of spectral lines. Such learning cannot be acquired from the automatic estimates provided by using …
Studying different scenarios of star formation in OB associations is crucial for understanding the structure and evolution of the Galaxy. The Canis Major OB1/R1 Association (CMa), in particular, hosts hundreds of young stars, and evidence indicates that at least three supernovae (SN) influenced its history. For these reasons, CMa serves as an ideal laboratory for investigating how superno…
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