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Bruno Mota
Researcher at Federal University of Rio de Janeiro
Publications - 74
Citations - 2066
Bruno Mota is an academic researcher from Federal University of Rio de Janeiro. The author has contributed to research in topics: Cosmic microwave background & Stars. The author has an hindex of 20, co-authored 68 publications receiving 1692 citations. Previous affiliations of Bruno Mota include University of São Paulo.
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Cellular scaling rules for rodent brains
TL;DR: It is proposed that the faster increase in average neuronal size in the cerebral cortex than in the cerebellum as these structures gain neurons and the rapidly increasing glial numbers that generate glial mass to match total neuronal mass at a fixed glia/neuron total mass ratio are fundamental cellular constraints that lead to the relative expansion of cerebral cortical volume across species.
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Cortical folding scales universally with surface area and thickness, not number of neurons
TL;DR: It is shown that the degree of cortical folding scales uniformly across lissencephalic and gyrencephalic species, across individuals, and within individual cortices as a function of the product of cortical surface area and the square root of cortical thickness.
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Connectivity-driven white matter scaling and folding in primate cerebral cortex
TL;DR: A white matter-based mechanism to account for increased cortical folding across species is offered, which is proposed to be driven by connectivity-related tension in the white matter, pulling down on the gray matter.
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Different scaling of white matter volume, cortical connectivity, and gyrification across rodent and primate brains
TL;DR: While the neuronal rules that govern gray and white matter scaling are different across rodents and primates, it is found that they can be explained by the same unifying model, with order-specific exponents.
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DYNAMICAL EVOLUTION OF VISCOUS DISKS AROUND Be STARS. I. PHOTOMETRY
Xavier Haubois,Xavier Haubois,Xavier Haubois,Bruno Mota,Alex C. Carciofi,Zachary H. Draper,Zachary H. Draper,John P. Wisniewski,D. Bednarski,Th. Rivinius +9 more
TL;DR: In this paper, the polarization color diagram (PCD) is used to track the dynamical phases of a Be star, such as disk build-up, dissipation, periodic, and episodic outbursts.