Not all stars are the Sun: rethinking the Mixing Length
Aula GrattonCharacterizing heat transport in stars is notoriously complicated, and the task of reproducing the physics
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Not all stars are the Sun: rethinking the Mixing Length
Aula GrattonCharacterizing heat transport in stars is notoriously complicated, and the task of reproducing the physics
Rossby number calculations for fully convective stars
Aula GrattonThe Rossby number is a quantity that gauges the relative importance of rotation in astrophysical
Rossby number calculations for fully convective stars
Aula GrattonThe Rossby number is a quantity that gauges the relative importance of rotation in astrophysical
Deep, multi-band photometry of low-mass stars to reveal young clusters: a blind study of the NGC 2264 region
Aula GrattonThe LSST survey will provide multi-epoch, multi-wavelength (u,g,r,i,z,y) mapping of the Southern Hemisphere, with a
Deep, multi-band photometry of low-mass stars to reveal young clusters: a blind study of the NGC 2264 region
Aula GrattonThe LSST survey will provide multi-epoch, multi-wavelength (u,g,r,i,z,y) mapping of the Southern Hemisphere, with a
Modern core-collapse supernova nucleosynthesis
Aula GrattonMassive stars and their core-collapse supernovae are key contributors to the evolution and chemical enrichment
Modern core-collapse supernova nucleosynthesis
Aula GrattonMassive stars and their core-collapse supernovae are key contributors to the evolution and chemical enrichment
The wee free magnetic elements on the photosphere: a turbulent story
Aula GrattonThe study of the dynamics of the photosphere allow us to investigate the physical processes
The wee free magnetic elements on the photosphere: a turbulent story
Aula GrattonThe study of the dynamics of the photosphere allow us to investigate the physical processes