Calendario di Eventi
L Lun
M Mar
M Mer
G Gio
V Ven
S Sab
D Dom
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
2 eventi,
0 eventi,
0 eventi,
2 eventi,
Not all stars are the Sun: rethinking the Mixing Length
Not all stars are the Sun: rethinking the Mixing Length
Characterizing heat transport in stars is notoriously complicated, and the task of reproducing the physics
Not all stars are the Sun: rethinking the Mixing Length
Not all stars are the Sun: rethinking the Mixing Length
Characterizing heat transport in stars is notoriously complicated, and the task of reproducing the physics
0 eventi,
0 eventi,
0 eventi,
2 eventi,
Rossby number calculations for fully convective stars
Rossby number calculations for fully convective stars
The Rossby number is a quantity that gauges the relative importance of rotation in astrophysical
Rossby number calculations for fully convective stars
Rossby number calculations for fully convective stars
The Rossby number is a quantity that gauges the relative importance of rotation in astrophysical
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
0 eventi,
2 eventi,
Deep, multi-band photometry of low-mass stars to reveal young clusters: a blind study of the NGC 2264 region
Deep, multi-band photometry of low-mass stars to reveal young clusters: a blind study of the NGC 2264 region
The 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
Deep, multi-band photometry of low-mass stars to reveal young clusters: a blind study of the NGC 2264 region
The LSST survey will provide multi-epoch, multi-wavelength (u,g,r,i,z,y) mapping of the Southern Hemisphere, with a
0 eventi,
2 eventi,
Modern core-collapse supernova nucleosynthesis
Modern core-collapse supernova nucleosynthesis
Massive stars and their core-collapse supernovae are key contributors to the evolution and chemical enrichment
Modern core-collapse supernova nucleosynthesis
Modern core-collapse supernova nucleosynthesis
Massive stars and their core-collapse supernovae are key contributors to the evolution and chemical enrichment
0 eventi,
0 eventi,
0 eventi,
0 eventi,
2 eventi,
The wee free magnetic elements on the photosphere: a turbulent story
The wee free magnetic elements on the photosphere: a turbulent story
The 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
The wee free magnetic elements on the photosphere: a turbulent story
The study of the dynamics of the photosphere allow us to investigate the physical processes