12 citations · 38 across the 9 of their papers we have counts for
12 papers
Light element abundances in carbon-enhanced metal-poor stars
Richard J. Stancliffe
We model the evolution of the abundances of light elements in carbon-enhanced metal-poor (CEMP) stars, under the assumption that such stars are formed by mass transfer in a binary…
Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
Richard J. Stancliffe, Evert Glebbeek
We investigate the formation of carbon-enhanced metal-poor (CEMP) stars via the scenario of mass transfer from a carbon-rich asymptotic giant branch (AGB) primary to a low-mass com…
Observing solar-like oscillations
Timothy R. Bedding, Hans Kjeldsen
The past few years have seen great progress in observing oscillations in solar-type stars, lying on or just above the main sequence. We review the most recent results, most of whic…
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…
Mass loss and supernova progenitors
John Eldridge
We first discuss the mass range of type IIP SN progenitors and how the upper and lower limits impose interesting constraints on stellar evolution. Then we discuss the possible impl…
Mass loss predictions for hot stars
Jorick S. Vink
I present the results of radiation-driven mass-loss predictions for hot stars of all mass. Mass loss is an important aspect for the evolution of massive stars, the rotational prope…