I have a bachelor's degree in Physics from the State University of Feira de Santana (UEFS) and a master's degree in Astronomy from the Institute of Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo (IAG/USP), with funding from FAPESP. In my master's degree, I studied a protostellar jet with non-thermal emission (synchrotron), located in a region of massive star formation, using data from the Karl G. Jansky Very Large Array (VLA) and interferometric analysis. Currently, in my doctorate, I investigate the different emission mechanisms present in protostellar jets, using high-resolution observations obtained with the VLA, the Atacama Large Millimeter/submillimeter Array (ALMA) and the Very Long Baseline Interferometry (VLBI) technique. I have experience in analyzing interferometric data and studying the physics of astrophysical jets. (Source: Lattes Curriculum)
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Astrophysical jets are energetic phenomena that are very present in astronomy. Their emission covers different scales, from young stars to supermassive black holes and active cores of galaxies. Jets are believed to play a central role in controlling mass accretion in protostars and black holes, as well as galaxy growth via AGN feedback; despite their importance, their formation mechanism …
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