2 citations · 2 across the 3 of their papers we have counts for
7 papers
Models of Stellar structure for asteroseismology
F. D'Antona, J. Montalban, I. Mazzitelli
Among the problems still open in the study of stellar structure, we discuss in particular some issues related to the study of convection. We have recently built up complete stellar…
To accrete or not to accrete: the dilemma of the recycling scenario
L. Burderi, F. D'Antona, T. Di Salvo +3
We study the evolution of a low-mass X-ray binary by coupling a binary stellar evolution code with a general relativistic code that describes the behaviour of the neutron star. We…
Radio ejection in the evolution of X-ray binaries: the bridge between low mass X-ray binaries and millisecond pulsars
Luciano Burderi, Francesca D'Antona, Tiziana Di Salvo +1
We present a scenario for the spin-up and evolution of binary millisecond pulsars. This can explain the observational properties of the recently discovered binary millisecond pulsa…
Old and new tools for understanding the evolution of stars in clusters
F. D'Antona
The uncertainties in the modelling of some important inputs of stellar evolution must be taken into account for a correct interpretation, both of the HR diagrams of individual star…
Where Have All the Submillisecond Pulsars Gone?
L. Burderi, F. D'Antona, M. T. Menna +8
The existence of pulsars with spin period below one millisecond is expected, though they have not been detected up to now. Their formation depends on the quantity of matter accrete…
The HR diagram of Globular Clusters: Theorist' view(s)
Francesca D'Antona
I list the characteristic features of Globular Cluster (GC) HR diagrams which provide a complete test of the stellar evolution of low mass stars: morphologies describing the differ…