Graduated in Astronomy at Universidade de São Paulo (2018). Obtained her MSc from Instituto de Astronomia, Geofísica e Ciências Atmosféricas, at Universidade de São Paulo (2020). Currently, is a PhD student in the Astronomy program at IAG-USP, and has as research interests the evolution of young low-mass stars - T Tauri stars - with an emphasis on heating mechanisms and angular moment transport in protostellar accretion disks. (Source: Lattes Curriculum)
| News published in Agência FAPESP Newsletter about the researcher |
| TITULO |
| Articles published in other media outlets (0 total): |
| More itemsLess items |
| VEICULO: TITULO (DATA) |
| VEICULO: TITULO (DATA) |
The angular momentum transport in accretion disks associated to young stellar objects is a key mechanism in understanding and describing the evolution of stars -and planetary systems- in their early stages. Currently, there are two important mechanisms used to describe the angular momentum transport in accretion disks of T Tauri stars: the Magnetorotational Instability (MRI) and the magne…
Accretion disks are commonly found around young stars, such as T Tauri stars. In order to occur the transport of matter to the star, the particles of the disk need to loose some of their rotational energy and fall towards the central object. The most promising mechanism of angular momentum transport is the magneto-rotational instability (IMR). However, this instability requires that the p…
Accretion disks are observed around young stars, as T Tauri stars. In order to have transport of disk material for the star it is necessary that the disk particles lose some of its rotational energy and "fall" toward the central object. The most promising angular momentum transport mechanism is the magneto-rotational instability (MRI). However, this instability requires that thegas partic…
| 1 / 1 | Ongoing scholarships in Brazil |
| 2 / 2 | Completed scholarships in Brazil |
| 3 / 3 | All Scholarships |
| Associated processes | |
CV Lattes
ORCID