Rossby number calculations for fully convective stars
Aula GrattonThe Rossby number is a quantity that gauges the relative importance of rotation in astrophysical
10 eventi found.
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
A Panchromatic View of High-Redshift Quasar Host Galaxies
Aula GrattonWhile it is now widely accepted that the growth of supermassive black-holes in galaxies is
A Panchromatic View of High-Redshift Quasar Host Galaxies
Aula GrattonWhile it is now widely accepted that the growth of supermassive black-holes in galaxies is