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An Explosive End to Intermediate-Mass Zero-Metallicity Stars and Early Universe Nucleosynthesis
H. B. Lau, R. J. Stancliffe, C. A. Tout
We use the Cambridge stellar evolution code STARS to model the evolution of 5-7 solar mass zero-metallicity stars. With enhanced resolution at the hydrogen and helium burning shell…
The effect of massive binaries on stellar populations and supernova progenitors
John J. Eldridge, Robert G. Izzard, Christopher A. Tout
We compare our latest single and binary stellar model results from the Cambridge STARS code to several sets of observations. We examine four stellar population ratios, the number o…
Impact of Rotation on the Evolution of Low-Mass Stars
D. Brown, M. Salaris, S. Cassisi +1
High precision photometry and spectroscopy of low-mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar…
The Impact of Rotation on the Evolution of Low-Mass Stars
D. Brown, M. Salaris
High precision photometry and spectroscopy of low-mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar…
The effect of different opacity data and chemical element mixture on the Petersen diagram
P. Lenz, A. A. Pamyatnykh, M. Breger
The Petersen diagram is a frequently used tool to constrain model parameters such as metallicity of radial double-mode pulsators. In this diagram the period ratio of the radial fir…
On the seismic age of the Sun
G. Houdek, D. O. Gough
We use low-degree acoustic modes obtained by the BiSON to estimate the main-sequence age of the Sun. The calibration is accomplished by linearizing the deviations from a…
Interacting Convection Zones
L. J. Silvers, M. R. E. Proctor
We present results from simulations to examine how the separation between two convectively unstable layers affect their interaction. We show that two convectively unstable layers r…
Alignment and Precession of a Black Hole with a Warped Accretion Disc
Rebecca G. Martin, J. E. Pringle, Christopher A. Tout
We consider the shape of an accretion disc whose outer regions are misaligned with the spin axis of a central black hole and calculate the steady state form of the warped disc in t…
Carbon Rich Extremely Metal Poor Stars: Signatures of Population-III AGB stars in Binary Systems
H. B. Lau, R. J. Stancliffe, C. A. Tout
We use the Cambridge stellar evolution code STARS to model the evolution and nucleosynthesis of zero-metallicity intermediate-mass stars. We investigate the effect of duplicity on…