Dust-driven stellar winds in stellar evolution models
Aula GrattonMass loss from stars during their evolution in the HR-diagram is an essential ingredient in
10 eventi found.
Dust-driven stellar winds in stellar evolution models
Aula GrattonMass loss from stars during their evolution in the HR-diagram is an essential ingredient in
The two-families scenario of compact stars: signatures and implications on GRBs
Aula GrattonIn the last years the possibility of discriminating between the various theoretically possible compositions of
The two-families scenario of compact stars: signatures and implications on GRBs
Aula GrattonIn the last years the possibility of discriminating between the various theoretically possible compositions of
Stellar evolution modeling of low-mass stars with magnetic fields: advances and challenges
Aula GrattonThough magnetic fields are commonly believed to play an important role on the structure and
Stellar evolution modeling of low-mass stars with magnetic fields: advances and challenges
Aula GrattonThough magnetic fields are commonly believed to play an important role on the structure and
The Milky Way bulge: chemical content, kinematics and 3D structure
Aula GrattonDuring the last decade large observational efforts have been focused on understanding the formation and
The Milky Way bulge: chemical content, kinematics and 3D structure
Aula GrattonDuring the last decade large observational efforts have been focused on understanding the formation and
Gas accretion and star formation in disk galaxies
Aula GrattonNumerical simulations predict that metal-poor gas accretion from the cosmic web fuels the formation of
Gas accretion and star formation in disk galaxies
Aula GrattonNumerical simulations predict that metal-poor gas accretion from the cosmic web fuels the formation of