High contrast imaging and the search for young exo-planets
Aula GrattonHigh contrast imaging has enormously progressed in the last twenty years, thanks to the development
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High contrast imaging and the search for young exo-planets
Aula GrattonHigh contrast imaging has enormously progressed in the last twenty years, thanks to the development
Dust Production from Evolved Stars in the Local Group
Aula GrattonInfrared observations of nearby galaxies and the Milky Way show that there are two main
Dust Production from Evolved Stars in the Local Group
Aula GrattonInfrared observations of nearby galaxies and the Milky Way show that there are two main
Microlensing
Aula GrattonI will review the microlensing and pixel lensing techniques and show how they play a
Microlensing
Aula GrattonI will review the microlensing and pixel lensing techniques and show how they play a
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
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